The nuclear reactions are very interesting and very big topic in research field, In this research paper we are describing about all types of nuclear reactions taking for light weight, medium weight and heavy
weight target nucleus, which is only one types of target nucleus.
Here our interest how many types nuclear reactions occur or don't occur at taking for light weight, medium weight and heavy weight target nucleus. Finding the reason why it doesn't become to taking other weight target nucleus and why it becomes in those types of targets nucleus. So we can say it can become very interesting topic in field of finding new information about nucleus reactions to taking different types of targets nucleus.
In the focus of attention at the present time are the new rare earth‐cobalt‐based magnet alloys. This paper is primarily a qualitative review of the physical phenomena controlling their behavior and of the materials problems these magnets have posed. It also provides an outlook at possibilities for the development of still better or cheaper permanent magnets which current research on rare earth‐ transition metal alloys appears to provide. The origins of the magnetic moments and the crystal anisotropy of rare earth‐transition metal phases are discussed. Alternative concepts of the causes of coercivity in powders and sintered bodies are analyzed. Some basic aspects of the sintering of R‐Co compacts and the magnetic hardening of R–Co–Cu alloys in the massive state are reviewed. Specific problems related to particular alloys and applications of the magnets are pointed out. The conclusion is drawn that the new family of permanent magnets now emerging rivals in complexity both the Alnicos and the ferrites together. There are many development opportunities for the future, and we can expect that, eventually, magnets based on high‐anisotropy alloys containing rare earths will be offered in a variety of grades, covering a wide range of properties and prices, and that they will be produced by several drastically different methods.
A session about nuclear engineering, made for public to increase the public awareness about nuclear energy, radiation, nuclear waste, and nuclear accidents
The Born-Haber cycle summarizes the standard enthalpy changes that occur during the formation of an ionic crystal from its gaseous constituent elements. It relates the standard enthalpy of sublimation, bond dissociation, electron affinity, and lattice energy to the standard enthalpy of atomization through Hess's law. For example, in forming NaCl, the standard enthalpy of atomization for sodium and chlorine contributes -411 kJ, which is balanced by the energy absorbed in ion formation, bond breaking, and crystal lattice formation.
The document discusses various types of nuclear reactions. It defines nuclear reactions as processes where two nuclei or nuclear particles collide and produce different products than the initial particles. It describes several types of nuclear reactions including elastic and inelastic scattering, pickup and stripping reactions, compound nuclear reactions, radioactive capture, and photo disintegration. Elastic scattering involves the projectile and outgoing particles being the same, while inelastic scattering results in a loss of energy and particles scattered in different directions with different energies. Pickup reactions involve a gain of nucleons from the target, and stripping reactions involve one or more nucleons captured from the projectile. The document provides examples of each type of reaction.
The document discusses nuclear chemistry and radioactivity. It describes how radioactive decay was discovered and the differences between nuclear and chemical reactions. It defines types of radiation like alpha, beta, and gamma rays. It also explains nuclear reactions, radioactive decay, half-lives, nuclear fission and fusion, and applications of nuclear chemistry like nuclear power generation and radiocarbon dating.
Ppt djy 2011 2 topic 7 and 13 nuclear reactionsDavid Young
This document provides an overview of atomic and nuclear physics topics 07 and 13, including:
1) Definitions of nuclear transmutations and artificial (induced) transmutations where a target nucleus is bombarded to cause a reaction.
2) Examples of common nuclear reactions and notations used.
3) Explanations of mass defect, binding energy, and binding energy per nucleon which help explain where the "missing mass" goes in nuclear reactions.
4) Descriptions of fusion and fission reactions where binding energy is released by combining or splitting nuclei.
Ajit Lulla has over 11 years of experience as a senior physics faculty. He previously taught at Allen Career Institute and has mentored many students who achieved top ranks in examinations like JEE and NEET, with some students achieving ranks as high as 69, 81, and 121. He holds a B.Tech degree from IIT Bombay and specializes in providing personalized guidance to students.
In the focus of attention at the present time are the new rare earth‐cobalt‐based magnet alloys. This paper is primarily a qualitative review of the physical phenomena controlling their behavior and of the materials problems these magnets have posed. It also provides an outlook at possibilities for the development of still better or cheaper permanent magnets which current research on rare earth‐ transition metal alloys appears to provide. The origins of the magnetic moments and the crystal anisotropy of rare earth‐transition metal phases are discussed. Alternative concepts of the causes of coercivity in powders and sintered bodies are analyzed. Some basic aspects of the sintering of R‐Co compacts and the magnetic hardening of R–Co–Cu alloys in the massive state are reviewed. Specific problems related to particular alloys and applications of the magnets are pointed out. The conclusion is drawn that the new family of permanent magnets now emerging rivals in complexity both the Alnicos and the ferrites together. There are many development opportunities for the future, and we can expect that, eventually, magnets based on high‐anisotropy alloys containing rare earths will be offered in a variety of grades, covering a wide range of properties and prices, and that they will be produced by several drastically different methods.
A session about nuclear engineering, made for public to increase the public awareness about nuclear energy, radiation, nuclear waste, and nuclear accidents
The Born-Haber cycle summarizes the standard enthalpy changes that occur during the formation of an ionic crystal from its gaseous constituent elements. It relates the standard enthalpy of sublimation, bond dissociation, electron affinity, and lattice energy to the standard enthalpy of atomization through Hess's law. For example, in forming NaCl, the standard enthalpy of atomization for sodium and chlorine contributes -411 kJ, which is balanced by the energy absorbed in ion formation, bond breaking, and crystal lattice formation.
The document discusses various types of nuclear reactions. It defines nuclear reactions as processes where two nuclei or nuclear particles collide and produce different products than the initial particles. It describes several types of nuclear reactions including elastic and inelastic scattering, pickup and stripping reactions, compound nuclear reactions, radioactive capture, and photo disintegration. Elastic scattering involves the projectile and outgoing particles being the same, while inelastic scattering results in a loss of energy and particles scattered in different directions with different energies. Pickup reactions involve a gain of nucleons from the target, and stripping reactions involve one or more nucleons captured from the projectile. The document provides examples of each type of reaction.
The document discusses nuclear chemistry and radioactivity. It describes how radioactive decay was discovered and the differences between nuclear and chemical reactions. It defines types of radiation like alpha, beta, and gamma rays. It also explains nuclear reactions, radioactive decay, half-lives, nuclear fission and fusion, and applications of nuclear chemistry like nuclear power generation and radiocarbon dating.
Ppt djy 2011 2 topic 7 and 13 nuclear reactionsDavid Young
This document provides an overview of atomic and nuclear physics topics 07 and 13, including:
1) Definitions of nuclear transmutations and artificial (induced) transmutations where a target nucleus is bombarded to cause a reaction.
2) Examples of common nuclear reactions and notations used.
3) Explanations of mass defect, binding energy, and binding energy per nucleon which help explain where the "missing mass" goes in nuclear reactions.
4) Descriptions of fusion and fission reactions where binding energy is released by combining or splitting nuclei.
Ajit Lulla has over 11 years of experience as a senior physics faculty. He previously taught at Allen Career Institute and has mentored many students who achieved top ranks in examinations like JEE and NEET, with some students achieving ranks as high as 69, 81, and 121. He holds a B.Tech degree from IIT Bombay and specializes in providing personalized guidance to students.
The document discusses nuclear chemistry and nuclear reactions. It defines nuclear chemistry as the study of nuclear changes in atoms, which are the source of radioactivity and nuclear power. There are two main types of nuclear reactions - artificial transmutation induced by bombarding atoms and natural transmutation that occurs spontaneously. Nuclear fission and fusion reactions are also described, where fission is the splitting of heavy nuclei and fusion is the combining of light nuclei. Key components of nuclear reactors like fuel, moderator, control rods and coolants are outlined. The document also discusses atomic bombs and how they work by achieving supercritical mass through compressing or combining subcritical masses. Applications of radioisotopes as tracers in chemical investigations are briefly mentioned.
Physics and Technology of Nuclear ReactorsPaul Callaghan
The following presentation was created by me (Paul Callaghan) in order to demonstrate learning on the Physics and Technology of Nuclear Reactors Course I attended from Autumn 2007 to Spring 2008 at The University of Birmingham.
This document discusses nuclear reactions and the formation of elements. It begins by explaining common types of nuclear reactions and providing examples of balancing nuclear equations. It then discusses nucleosynthesis during the Big Bang, in stars, and during supernovas. Big Bang nucleosynthesis produced hydrogen and helium. In stars, nuclear fusion of light elements produces heavier elements up to iron. During supernovas, rapid and slow neutron capture processes produce elements heavier than iron. The document concludes with timelines showing the development of atomic theory from ancient Greek philosophers to modern scientists like Rutherford, Bohr and Moseley.
L8 Introduction to Reactor Physics Part 1.pdfRHOWELLETIBAY1
- The document provides an introduction to reactor physics concepts including neutron interactions, nuclear cross sections, reaction rates, neutron moderation, and neutron attenuation.
- It describes various neutron interactions such as elastic scattering, inelastic scattering, radiative capture, charge production, neutron production, and fission. Microscopic and macroscopic cross sections, and their relationship to reaction rates are also covered.
- The concepts of neutron moderation, thermalization, and the role of moderators are summarized. An ideal moderator is described as having a large scattering cross section, small absorption cross section, and large energy loss per collision.
This document discusses nucleophilic substitution reactions, specifically SN1 and SN2 mechanisms. It defines the key aspects of each mechanism, including:
- SN2 is a concerted, one-step mechanism where nucleophilic attack and bond cleavage occur simultaneously. It results in inversion of configuration.
- SN1 is a two-step mechanism involving a carbocation intermediate. Both enantiomers may be produced. Stereochemistry is not inverted.
- Factors like the nature of the nucleophile and leaving group, carbocation stability, and substrate structure determine whether a reaction will proceed by SN1 or SN2.
The document discusses nuclear chemistry concepts including isotopes, nuclear reactions, radioactive decay via alpha, beta, and gamma emission, and the effects of radiation exposure. It provides examples of nuclear equations to represent different types of radioactive decay and nuclear reactions. The document also explains different nuclear particles like neutrons, protons, electrons, positrons, and alpha particles that are involved in nuclear reactions and radioactive decay.
Nuclear physics is a branch of physics that focuses on the study of atomic nuclei and their interactions. It explores the properties and behavior of atomic nuclei, which are the central cores of atoms containing protons and neutrons. This field is crucial for understanding the fundamental forces that govern the behavior of matter at the atomic and subatomic levels.
02. ch32 (ionizing radiation, nuclear energy, and elementary particles)Diajeng Ramadhan
Ionizing radiation consists of photons and/or moving particles that have sufficient energy to knock electrons out of atoms. Exposure measures radiation produced in air, while absorbed dose measures the energy absorbed from radiation per unit mass of material. Relative biological effectiveness compares the biological damage of different types of radiation, and biologically equivalent dose is the product of absorbed dose and RBE. Nuclear reactions occur when incident particles or photons cause changes in target nuclei, such as uranium transmuting into plutonium. Nuclear fission occurs when a slow neutron splits a heavy nucleus like uranium into lighter elements, and a controlled chain reaction in a nuclear reactor uses fuel, control rods, and a moderator.
1. Photochemistry is the study of chemical reactions caused by the absorption of light. It involves photochemical reactions, which require light for initiation, as well as photophysical processes during the de-excitation of excited molecules.
2. Key concepts in photochemistry include Grotthuss-Draper law, Lambert's law, Beer's law, and Stark-Einstein law of photochemical equivalence. Quantum yield determines the efficiency of photochemical reactions.
3. Photochemistry examines differences between photochemical and thermal reactions. It also explores photochemical processes like fluorescence, phosphorescence, internal conversion, and intersystem crossing depicted in Jablonski diagrams.
Types Of nuclear reactions. Nuclear Fission Reaction. Nuclear Fusion Reaction. Difference between nuclear fusion and nuclear fusion. Light Element Fission. Light Element Fusion. Nuclear Fusion on Sun. Beta Decay process happening in sun. A short explanation of D–D reaction, D–He(3) reaction, D–T reaction. the outstanding problem is the tritium supply. Binding energy curve.Energy partition in process of fusion reactions. How then can light element fusion reactions be initiated? A major explanation for all these above steps. A complete explanation by Syed Hammad Ali Gillani.
Nuclear physics studies the building blocks and interactions of atomic nuclei. The field is the basis for applications like nuclear power, nuclear bombs, nuclear medicine, and radiocarbon dating. Atoms consist of a nucleus containing protons and neutrons, surrounded by orbiting electrons. Radioactivity occurs when unstable atomic nuclei decay by emitting particles like alpha and beta particles or gamma rays. Nuclear fission and fusion can release energy as nuclei split or combine.
The document discusses several key concepts regarding nuclear energy including:
1) Atomic structure including atomic number, mass number, and isotopes.
2) Nuclear reactions and equations including conservation of nucleons and factors that affect neutron multiplication.
3) Energy released from nuclear fission including the total energy of about 200 MeV per fission and the breakdown of energy types.
4) Radioactivity and the different types of decay including alpha, beta, gamma, positron, neutron emission, and half-life.
Nuclear physics is the study of atomic nuclei and their components. It includes properties of the nucleus, particles within it like protons and neutrons, and their interactions. Key topics covered are radioactivity, nuclear reactions like fission and fusion, and practical applications. Fission is the splitting of large nuclei into smaller ones and is used in nuclear reactors to generate controlled energy. Fusion is the combining of small nuclei into larger ones and produces even more energy but is difficult to control.
This document discusses nucleophilic substitution reactions. It begins by defining nucleophiles as negatively charged ions or neutral molecules with a lone pair of electrons. It then explains the mechanisms of the SN2 and SN1 reactions. The SN2 is a concerted bimolecular reaction where the nucleophile attacks from the backside of the substrate, inverting the configuration. The SN1 is a unimolecular reaction that proceeds through a carbocation intermediate, allowing for retention or inversion of configuration. Finally, it discusses factors like temperature, nucleophile strength, and substrate structure that determine whether a reaction will proceed by SN1 or SN2.
Nuclear physics describes the structure and interactions of atomic nuclei. Rutherford discovered the nucleus through alpha scattering experiments. Protons and neutrons were later identified. Isotopes have the same number of protons but different numbers of neutrons. Mass defect and binding energy explain why atomic nuclei are more stable than separated nucleons. Radioactive decay occurs spontaneously at a rate proportional to the number of unstable nuclei. Exponential decay and half-life are described by the decay constant. Nuclear reactions conserve nucleon number and charge. Energy is released or absorbed through mass-energy equivalence. Fission and fusion occur under different conditions according to binding energy. Controlled fission in reactors uses moderation and feedback to sustain a chain reaction. Fusion
Nuclear energy is emitted from radioactive elements during nuclear fission or fusion reactions. Nuclear fission involves splitting heavy radioactive nuclei, while nuclear fusion combines lighter nuclei. Fission is used in nuclear power plants to generate electricity through controlled chain reactions, using elements like uranium. Fusion occurs in stars and requires extremely high temperatures. While nuclear energy produces less waste than fossil fuels, the byproducts are radioactive and require careful treatment or storage due to their harmfulness.
Photochemistry is the study of chemical reactions caused by the absorption of visible or ultraviolet light. There are two main types of reactions: primary processes where light is directly absorbed, and secondary processes involving excited states produced in primary processes. Factors like fluorescence, quantum yield, and chain reactions can affect the efficiency of photochemical reactions. Photochemistry plays roles in important natural and industrial processes.
This document discusses three types of nuclear reactions: radioactive decay, fission, and fusion. Radioactive decay occurs when an unstable isotope emits particles and becomes more stable. Fission involves a heavy nucleus splitting into lighter nuclei. Fusion is when two nuclei merge to form a heavier nucleus. Nuclear reactions are over 1 million times more powerful than chemical reactions because a small amount of mass can be converted to a large amount of energy according to Einstein's equation E=mc2.
Pericyclic reactions involve the formation or breaking of bonds in a cyclic transition state. They include cycloadditions, electrocyclic reactions, sigmatropic rearrangements, and others. Cycloadditions like the Diels-Alder reaction involve the combination of unsaturated molecules to form a cyclic adduct. The Diels-Alder reaction between a conjugated diene and dienophile forms a cyclohexene ring. Frontier molecular orbital theory can explain the regioselectivity of cycloadditions. Examples of pericyclic reactions include the synthesis of citral via a Claisen rearrangement, Fischer indole synthesis, and Diels-Alder reactions in alkaloid and carbohydrate synthesis.
New Thermodynamics: A Superior Fit Revised Kinetic Theoryijrap
The accepted kinetic theory forms a basis for modern thermodynamics and is mathematically based upon equipartition and degrees of freedom. It remains plagued with the necessity of numerous degrees of freedom exceptions for it to explain both empirically determined heat capacities and adiabatic indexes. Furthermore, assuming kT/2 per degree of freedom is to accept that a gas molecule possesses a specified energy without providing any clarity concerning that energy’s origins. Energy without an origin contravenes the first law of thermodynamics. This author’s previously published superior fit kinetic theory will be clarified and elaborated upon. This includes showing that this revised kinetic theory is a superior fit to both known heat capacities and adiabatic indexes. Not only is it a superior fit that does not rely upon any exceptions, this author’s kinetic theory also provides insight into the actual sources of a gas molecule’s energy. Furthermore, clarity concerning the difference between isometric (isochoric) and isobaric heat capacities in terms of sensible work will be discussed, along withits likely empirical verification.
On the Unification of Physic and the Elimination of Unbound Quantitiesijrap
This paper supports Descartes' idea of a constant quantity of motion, modernized by Leibniz. Unlike Leibniz, the paper emphasizes that the idea is not realized by forms of energy, but by energy itself. It remains constant regardless of the form, type, or speed of motion, even that of light. Through force, energy is only transformed. Here it is proved that force is its derivative. It exists even at rest, representing the object's minimal energy state. With speed, we achieve its multiplication up to the maximum energy state, from which a maximum force is derived from the object. From this point, corresponding to Planck's Length, we find the value of the force wherever we want. Achieving this removes the differences between various natural forces. The new idea eliminates infinite magnitudes. The process allows the laws to transition from simple to complex forms and vice versa, through differentiation-integration. For this paper, this means achieving the Unification Theory.
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Similar to Nuclear Reaction Taking Different Weight Target Nucleus
The document discusses nuclear chemistry and nuclear reactions. It defines nuclear chemistry as the study of nuclear changes in atoms, which are the source of radioactivity and nuclear power. There are two main types of nuclear reactions - artificial transmutation induced by bombarding atoms and natural transmutation that occurs spontaneously. Nuclear fission and fusion reactions are also described, where fission is the splitting of heavy nuclei and fusion is the combining of light nuclei. Key components of nuclear reactors like fuel, moderator, control rods and coolants are outlined. The document also discusses atomic bombs and how they work by achieving supercritical mass through compressing or combining subcritical masses. Applications of radioisotopes as tracers in chemical investigations are briefly mentioned.
Physics and Technology of Nuclear ReactorsPaul Callaghan
The following presentation was created by me (Paul Callaghan) in order to demonstrate learning on the Physics and Technology of Nuclear Reactors Course I attended from Autumn 2007 to Spring 2008 at The University of Birmingham.
This document discusses nuclear reactions and the formation of elements. It begins by explaining common types of nuclear reactions and providing examples of balancing nuclear equations. It then discusses nucleosynthesis during the Big Bang, in stars, and during supernovas. Big Bang nucleosynthesis produced hydrogen and helium. In stars, nuclear fusion of light elements produces heavier elements up to iron. During supernovas, rapid and slow neutron capture processes produce elements heavier than iron. The document concludes with timelines showing the development of atomic theory from ancient Greek philosophers to modern scientists like Rutherford, Bohr and Moseley.
L8 Introduction to Reactor Physics Part 1.pdfRHOWELLETIBAY1
- The document provides an introduction to reactor physics concepts including neutron interactions, nuclear cross sections, reaction rates, neutron moderation, and neutron attenuation.
- It describes various neutron interactions such as elastic scattering, inelastic scattering, radiative capture, charge production, neutron production, and fission. Microscopic and macroscopic cross sections, and their relationship to reaction rates are also covered.
- The concepts of neutron moderation, thermalization, and the role of moderators are summarized. An ideal moderator is described as having a large scattering cross section, small absorption cross section, and large energy loss per collision.
This document discusses nucleophilic substitution reactions, specifically SN1 and SN2 mechanisms. It defines the key aspects of each mechanism, including:
- SN2 is a concerted, one-step mechanism where nucleophilic attack and bond cleavage occur simultaneously. It results in inversion of configuration.
- SN1 is a two-step mechanism involving a carbocation intermediate. Both enantiomers may be produced. Stereochemistry is not inverted.
- Factors like the nature of the nucleophile and leaving group, carbocation stability, and substrate structure determine whether a reaction will proceed by SN1 or SN2.
The document discusses nuclear chemistry concepts including isotopes, nuclear reactions, radioactive decay via alpha, beta, and gamma emission, and the effects of radiation exposure. It provides examples of nuclear equations to represent different types of radioactive decay and nuclear reactions. The document also explains different nuclear particles like neutrons, protons, electrons, positrons, and alpha particles that are involved in nuclear reactions and radioactive decay.
Nuclear physics is a branch of physics that focuses on the study of atomic nuclei and their interactions. It explores the properties and behavior of atomic nuclei, which are the central cores of atoms containing protons and neutrons. This field is crucial for understanding the fundamental forces that govern the behavior of matter at the atomic and subatomic levels.
02. ch32 (ionizing radiation, nuclear energy, and elementary particles)Diajeng Ramadhan
Ionizing radiation consists of photons and/or moving particles that have sufficient energy to knock electrons out of atoms. Exposure measures radiation produced in air, while absorbed dose measures the energy absorbed from radiation per unit mass of material. Relative biological effectiveness compares the biological damage of different types of radiation, and biologically equivalent dose is the product of absorbed dose and RBE. Nuclear reactions occur when incident particles or photons cause changes in target nuclei, such as uranium transmuting into plutonium. Nuclear fission occurs when a slow neutron splits a heavy nucleus like uranium into lighter elements, and a controlled chain reaction in a nuclear reactor uses fuel, control rods, and a moderator.
1. Photochemistry is the study of chemical reactions caused by the absorption of light. It involves photochemical reactions, which require light for initiation, as well as photophysical processes during the de-excitation of excited molecules.
2. Key concepts in photochemistry include Grotthuss-Draper law, Lambert's law, Beer's law, and Stark-Einstein law of photochemical equivalence. Quantum yield determines the efficiency of photochemical reactions.
3. Photochemistry examines differences between photochemical and thermal reactions. It also explores photochemical processes like fluorescence, phosphorescence, internal conversion, and intersystem crossing depicted in Jablonski diagrams.
Types Of nuclear reactions. Nuclear Fission Reaction. Nuclear Fusion Reaction. Difference between nuclear fusion and nuclear fusion. Light Element Fission. Light Element Fusion. Nuclear Fusion on Sun. Beta Decay process happening in sun. A short explanation of D–D reaction, D–He(3) reaction, D–T reaction. the outstanding problem is the tritium supply. Binding energy curve.Energy partition in process of fusion reactions. How then can light element fusion reactions be initiated? A major explanation for all these above steps. A complete explanation by Syed Hammad Ali Gillani.
Nuclear physics studies the building blocks and interactions of atomic nuclei. The field is the basis for applications like nuclear power, nuclear bombs, nuclear medicine, and radiocarbon dating. Atoms consist of a nucleus containing protons and neutrons, surrounded by orbiting electrons. Radioactivity occurs when unstable atomic nuclei decay by emitting particles like alpha and beta particles or gamma rays. Nuclear fission and fusion can release energy as nuclei split or combine.
The document discusses several key concepts regarding nuclear energy including:
1) Atomic structure including atomic number, mass number, and isotopes.
2) Nuclear reactions and equations including conservation of nucleons and factors that affect neutron multiplication.
3) Energy released from nuclear fission including the total energy of about 200 MeV per fission and the breakdown of energy types.
4) Radioactivity and the different types of decay including alpha, beta, gamma, positron, neutron emission, and half-life.
Nuclear physics is the study of atomic nuclei and their components. It includes properties of the nucleus, particles within it like protons and neutrons, and their interactions. Key topics covered are radioactivity, nuclear reactions like fission and fusion, and practical applications. Fission is the splitting of large nuclei into smaller ones and is used in nuclear reactors to generate controlled energy. Fusion is the combining of small nuclei into larger ones and produces even more energy but is difficult to control.
This document discusses nucleophilic substitution reactions. It begins by defining nucleophiles as negatively charged ions or neutral molecules with a lone pair of electrons. It then explains the mechanisms of the SN2 and SN1 reactions. The SN2 is a concerted bimolecular reaction where the nucleophile attacks from the backside of the substrate, inverting the configuration. The SN1 is a unimolecular reaction that proceeds through a carbocation intermediate, allowing for retention or inversion of configuration. Finally, it discusses factors like temperature, nucleophile strength, and substrate structure that determine whether a reaction will proceed by SN1 or SN2.
Nuclear physics describes the structure and interactions of atomic nuclei. Rutherford discovered the nucleus through alpha scattering experiments. Protons and neutrons were later identified. Isotopes have the same number of protons but different numbers of neutrons. Mass defect and binding energy explain why atomic nuclei are more stable than separated nucleons. Radioactive decay occurs spontaneously at a rate proportional to the number of unstable nuclei. Exponential decay and half-life are described by the decay constant. Nuclear reactions conserve nucleon number and charge. Energy is released or absorbed through mass-energy equivalence. Fission and fusion occur under different conditions according to binding energy. Controlled fission in reactors uses moderation and feedback to sustain a chain reaction. Fusion
Nuclear energy is emitted from radioactive elements during nuclear fission or fusion reactions. Nuclear fission involves splitting heavy radioactive nuclei, while nuclear fusion combines lighter nuclei. Fission is used in nuclear power plants to generate electricity through controlled chain reactions, using elements like uranium. Fusion occurs in stars and requires extremely high temperatures. While nuclear energy produces less waste than fossil fuels, the byproducts are radioactive and require careful treatment or storage due to their harmfulness.
Photochemistry is the study of chemical reactions caused by the absorption of visible or ultraviolet light. There are two main types of reactions: primary processes where light is directly absorbed, and secondary processes involving excited states produced in primary processes. Factors like fluorescence, quantum yield, and chain reactions can affect the efficiency of photochemical reactions. Photochemistry plays roles in important natural and industrial processes.
This document discusses three types of nuclear reactions: radioactive decay, fission, and fusion. Radioactive decay occurs when an unstable isotope emits particles and becomes more stable. Fission involves a heavy nucleus splitting into lighter nuclei. Fusion is when two nuclei merge to form a heavier nucleus. Nuclear reactions are over 1 million times more powerful than chemical reactions because a small amount of mass can be converted to a large amount of energy according to Einstein's equation E=mc2.
Pericyclic reactions involve the formation or breaking of bonds in a cyclic transition state. They include cycloadditions, electrocyclic reactions, sigmatropic rearrangements, and others. Cycloadditions like the Diels-Alder reaction involve the combination of unsaturated molecules to form a cyclic adduct. The Diels-Alder reaction between a conjugated diene and dienophile forms a cyclohexene ring. Frontier molecular orbital theory can explain the regioselectivity of cycloadditions. Examples of pericyclic reactions include the synthesis of citral via a Claisen rearrangement, Fischer indole synthesis, and Diels-Alder reactions in alkaloid and carbohydrate synthesis.
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New Thermodynamics: A Superior Fit Revised Kinetic Theoryijrap
The accepted kinetic theory forms a basis for modern thermodynamics and is mathematically based upon equipartition and degrees of freedom. It remains plagued with the necessity of numerous degrees of freedom exceptions for it to explain both empirically determined heat capacities and adiabatic indexes. Furthermore, assuming kT/2 per degree of freedom is to accept that a gas molecule possesses a specified energy without providing any clarity concerning that energy’s origins. Energy without an origin contravenes the first law of thermodynamics. This author’s previously published superior fit kinetic theory will be clarified and elaborated upon. This includes showing that this revised kinetic theory is a superior fit to both known heat capacities and adiabatic indexes. Not only is it a superior fit that does not rely upon any exceptions, this author’s kinetic theory also provides insight into the actual sources of a gas molecule’s energy. Furthermore, clarity concerning the difference between isometric (isochoric) and isobaric heat capacities in terms of sensible work will be discussed, along withits likely empirical verification.
On the Unification of Physic and the Elimination of Unbound Quantitiesijrap
This paper supports Descartes' idea of a constant quantity of motion, modernized by Leibniz. Unlike Leibniz, the paper emphasizes that the idea is not realized by forms of energy, but by energy itself. It remains constant regardless of the form, type, or speed of motion, even that of light. Through force, energy is only transformed. Here it is proved that force is its derivative. It exists even at rest, representing the object's minimal energy state. With speed, we achieve its multiplication up to the maximum energy state, from which a maximum force is derived from the object. From this point, corresponding to Planck's Length, we find the value of the force wherever we want. Achieving this removes the differences between various natural forces. The new idea eliminates infinite magnitudes. The process allows the laws to transition from simple to complex forms and vice versa, through differentiation-integration. For this paper, this means achieving the Unification Theory.
Gravity Also Redshifts Light – the Missing Phenomenon That Could Resolve Most...ijrap
In this paper I discover that gravity also redshifts light like the velocity of its source does. When light travels towards a supermassive object, its waves (or photons) undergo continuous stretching, thereby shifting towards lower frequencies. Gravity redshifts light irrespective of whether its source is in motion or static with respect to its observer. An equation is derived for gravitational redshift, and a formula for combined redshift is presented by considering both the velocity, and gravity redshifts. Also explained is how frequencies of electromagnetic spectrum continuously downgrade as a light beam of mix frequencies passes towards a black hole. Further, a clear methodology is provided to figure out whether expansion of the universe is accelerating or decelerating, or alternatively, the universe is contracting.
In this paper I present a new theory that explains as to when and how dark energy is created as mass is destroyed. The theory extends Einstein’s mass energy equation to a more generic form in order to make it work even in high gravity conditions. It also explains why dark energy is created. Further, it is proved Einstein’s mass energy equation holds good only when the destroyed mass has no supermassive object in its close vicinity. The relationship between dark energy and dark matter is unveiled. An extended mathematical form of Einstein’s mass energy equation is derived, based on which the conditions leading to dark energy creation are explained. Three new physical parameters called dark energy discriminant, dark energy radius and dark energy boundary are introduced to facilitate easy understanding of the theory. It is explained in detail that an extremely superdense object has two dark energy boundaries, outer and inner. Mass destroyed only between these two boundaries creates dark energy. Dark energy space, the space between the two aforementioned boundaries, shrouds visible matter in obscurity from optical and electromagnetic telescopes. This theory identifies Gargantuan as a superdense black hole currently creating fresh dark energy, which could be the subject of interest for the astronomical research community having access to sophisticated telescopes, and working on dark energy. It also upholds dark energy and denies the existence of dark matter. Dark matter is nothing but the well-known visible matter positioned in dark energy space. An important relationship is derived between a photon’s frequency and its distance from a black hole to demonstrate the effect of gravity on light. Another important fact revealed by this theory is gravity stretches out light, thereby causing redshift, which is unaccounted in the computation of velocities of outer galaxies. Whether the universe is undergoing accelerated or decelerated expansion, or accelerated contraction can precisely be determined only after accounting for the redshift caused by gravity
International Journal on Soft Computing, Artificial Intelligence and Applicat...ijrap
International Journal on Soft Computing, Artificial Intelligence and Applications (IJSCAI)
is an open access peer-reviewed journal that provides an excellent international forum for sharing
knowledge and results in theory, methodology and applications of Artificial Intelligence, Soft
Computing. The Journal looks for significant contributions to all major fields of the Artificial
Intelligence, Soft Computing in theoretical and practical aspects. The aim of the Journal is to
provide a platform to the researchers and practitioners from both academia as well as industry to
meet and share cutting-edge development in the field.
Authors are solicited to contribute to the journal by submitting articles that illustrate research
results, projects, surveying works and industrial experiences that describe significant advances in
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SOME THEORETICAL ASPECTS OF HYDROGEN DIFFUSION IN BCC METALS AT LOW TEMPERATURESijrap
Purpose of the work is to discuss some theoretical aspects of the diffusion of hydrogen atoms in the crystal
lattice of BCC metals at low temperatures using the methods of statistical thermodynamics. The values of
the statistical model calculations of H diffusion coefficients in α-Fe, V, Ta, Nb, K are in good agreement
with the experimental data. The statistical model can also explain deviations from the Arrhenius equation
at temperatures 300-100 K in α-Fe, V, Nb and K. It was suggested that thermally activated fast tunnelling
transition of hydrogen atoms through the potential barrier at a temperature below 300 K provides an
almost free movement of H atoms in the α-Fe and V lattice at these temperatures. The results show that
quantum-statistical effects play a decisive role in the H diffusion in BCC metals at low temperatures. Using
the statistical model allows for the prediction of the diffusion coefficient for H in BCC metals at low
temperatures, where it’s necessary to consider quantum effects.
MASSIVE PHOTON HYPOTHESIS OPENS DOORS TO NEW FIELDS OF RESEARCHijrap
1) A massive photon hypothesis is proposed, where the photon mass is directly calculated from kinetic gas theory to be 1.25605 x 10-39 kg.
2) This photon mass explains various experiments like light deflection near the Sun and the gravitational redshift.
3) The photon gas is found to behave as a perfect blackbody and ideal gas, with photons having 6 degrees of freedom.
4) The thermal de Broglie wavelength of this photon gas is calculated to be 1.75967 x 10-3 m, matching the wavelength of the cosmic microwave background radiation.
5) This links the CMB radiation to being continuously generated by the photon gas permeating space, rather than being a relic of
PHENOMENOLOGICAL METHOD REGARDING A THIRD THEORY OF PHYSICS “THE EVENT:THE TH...ijrap
The quest for a third theory uniting macro-cosmos (relativity) and micro-cosmos (quantum mechanics) has coexisted with the denial of feminine/subjective polarity to masculine/objective. The dismissal of electromagnetism as the tension of opposites in quest of inner/outer unity is sourced in the denial of the feminine qualia -- the negative force field attributed to dark energy/dark matter. However, a conversion philosophy sourced in the hieros gamos and signified by the Mobius strip has formulated an integral consciousness methodology producing quantum objects by means of embracing the shadow haunting contemporary physics. This Self-reflecting process integrating subject/object comprises an ontology of kairos as the “quantum leap.” An interdisciplinary quest to create a phenomenological narrative is disclosed via a holistic apparatus of hermeneutics manifesting image/text of a contemporary grail journey. Reflected in this Third space is the sacred reality of autonomous number unifying polarities of feminine/subjective (quality) and objective/masculine (quantity) as new measurement apparatus for the quantum wave collapse.
3rd International Conference on Integrating Technology in Education (ITE 2022)ijrap
3rd International Conference on Integrating Technology in Education (ITE 2022) This forum also aims to provide a platform for exchanging ideas in new emerging trends that needs more focus and exposure and will attempt to publish proposals that strengthen our goals.
A SPECIAL RELATIONSHIP BETWEEN MATTER, ENERGY, INFORMATION, AND CONSCIOUSNESSijrap
This paper discusses the advantages of describing the universe, or nature, in terms of information and consciousness. Some problems encountered by theoretical physicists in the quest for the theory of everything stem from the limitations of trying to understand everything in terms of matter and energy only. However, if everything, including matter, energy, life, and mental processes, is described in terms of information and consciousness, much progress can be made in the search for the ultimate theory of the universe. As brilliant and successful as physics and chemistry have been over the last two centuries, it is important that nature is not viewed solely in terms of matter and energy. Two additional components are needed to unlock her secrets. While extensive writing exists that describes the connection between matter and energy and their physical basis, little work has been done to learn the special relationship between matter, energy, information, and consciousness.
This paper discusses the advantages of describing the universe, or nature, in terms of information and consciousness. Some problems encountered by theoretical physicists in the quest for the theory of everything stem from the limitations of trying to understand everything in terms of matter and energy only. However, if everything, including matter, energy, life, and mental processes, is described in terms of information and consciousness, much progress can be made in the search for the ultimate theory of the universe. As brilliant and successful as physics and chemistry have been over the last two centuries, it is important that nature is not viewed solely in terms of matter and energy. Two additional components are needed to unlock her secrets. While extensive writing exists that describes the connection between matter and energy and their physical basis, little work has been done to learn the special relationship between matter, energy, information, and
consciousness.
THE CONCEPT OF SPACE AND TIME: AN AFRICAN PERSPECTIVEijrap
Understanding the concept of space and time is critical, essential, and fundamental in searching for theall-encompassing theory or the theory of everything (ToE). Some physicists argue that time exists, whileothers posit that time is only a social or mental construct. The author presents an African thought systemon space and time conception, focusing on the African (Bantu) view of space and time. The author arguesthat before the advent of the Western linear view of space and time, Africans had their own visionregarding these two concepts. Their conception of time appears to be holistic, highly philosophical, non-linear, and thought-provoking. The author hopes that exploring these two concepts from an African perspective will provide a new and more in-depth insight into reality's nature. A scientific investigation of space and time from an African-centered perspective is a worthy and necessary endeavor in the quest forthe ToE
Learning to Pronounce as Measuring Cross Lingual Joint Orthography Phonology ...ijrap
Machine learning models allow us to compare languages by showing how hard a task in each language might be to learn and perform well on. Following this line of investigation, we explore what makes a language “hard to pronounce” by modelling the task of grapheme-to-phoneme (g2p) transliteration. By training a character-level transformer model on this task across 22 languages and measuring the model’s proficiency against its grapheme and phoneme inventories, we show that certain characteristics emerge that separate easier and harder languages with respect to learning to pronounce. Namely the complexity of a language's pronunciation from its orthography is due to the expressive or simplicity of its grapheme-to phoneme mapping. Further discussion illustrates how future studies should consider relative data sparsity per language to design fairer cross-lingual comparison tasks.
THE CONCEPT OF SPACE AND TIME: AN AFRICAN PERSPECTIVEijrap
Understanding the concept of space and time is critical, essential, and fundamental in searching for the all-encompassing theory or the theory of everything (ToE). Some physicists argue that time exists, while others posit that time is only a social or mental construct. The author presents an African thought system on space and time conception, focusing on the African (Bantu) view of space and time. The author argues
that before the advent of the Western linear view of space and time, Africans had their own vision
regarding these two concepts. Their conception of time appears to be holistic, highly philosophical, nonlinear, and thought-provoking. The author hopes that exploring these two concepts from an African
perspective will provide a new and more in-depth insight into reality's nature. A scientific investigation of space and time from an African-centered perspective is a worthy and necessary endeavor in the quest for the ToE.
International Journal of Recent advances in Physics (IJRAP)ijrap
International Journal of Recent advances in Physics (IJRAP) is a peer-reviewed, open access journal, addresses the impacts and challenges of Physics. The journal documents practical and theoretical results which make a fundamental contribution for the development of Physics.
The Concept of Space and Time: An African Perspectiveijrap
Understanding the concept of space and time is critical, essential, and fundamental in searching for the all-encompassing theory or the theory of everything (ToE). Some physicists argue that time exists, while others posit that time is only a social or mental construct. The author presents an African thought system on space and time conception, focusing on the African (Bantu) view of space and time. The author argues that before the advent of the Western linear view of space and time, Africans had their own vision regarding these two concepts. Their conception of time appears to be holistic, highly philosophical, nonlinear, and thought-provoking. The author hopes that exploring these two concepts from an African perspective will provide a new and more in-depth insight into reality's nature. A scientific investigation of space and time from an African-centered perspective is a worthy and necessary endeavor in the quest for the ToE.
The majority of physicists take it for granted that the universe is made up of matter. In turn, matter is composed of atoms; atoms are made up of particles such as electrons, protons, neutrons, etc. Also, protons
and neutrons are composed of quarks, etc. Furthermore, that everything in nature is governed by the known laws of physics and chemistry. The author only partially shares this view. He argues that many phenomena in the universe may depend on rules or factors as yet incorporated by the physical sciences.
The last few years have led him to reflect on the many unsolved physics problems, such as the quest for the theory of everything (ToE), the arrow of time, the interpretation of quantum mechanics, the fine-tuned
universe, etc. to mention just a few. The author posits that a field carries information, performs various mathematical and computational operations, and behaves as an intelligent entity embedded with consciousness.
Call For Papers - International Journal of Recent advances in Physics (IJRAP)ijrap
International Journal of Recent advances in Physics (IJRAP) is a peer-reviewed, open access journal, addresses the impacts and challenges of Physics. The journal documents practical and theoretical results which make a fundamental contribution for the development of Physics.
Call For Papers - International Journal of Recent advances in Physics (IJRAP)ijrap
The International Journal of Recent Advances in Physics (IJRAP) is a peer-reviewed open access journal that addresses impacts and challenges in the field of physics. It covers theoretical and practical results across many areas of physics including advanced functional materials, applied optics, condensed matter physics, nuclear physics, quantum physics, and more. Authors are invited to submit papers by email before October 30, 2021. Notifications of acceptance will be provided by November 25, 2021.
Call For Papers - International Journal of Recent advances in Physics (IJRAP)ijrap
International Journal of Recent advances in Physics (IJRAP) is a peer-reviewed, open access journal, addresses the impacts and challenges of Physics. The journal documents practical and theoretical results which make a fundamental contribution for the development of Physics.
Discovery of An Apparent Red, High-Velocity Type Ia Supernova at 𝐳 = 2.9 wi...Sérgio Sacani
We present the JWST discovery of SN 2023adsy, a transient object located in a host galaxy JADES-GS
+
53.13485
−
27.82088
with a host spectroscopic redshift of
2.903
±
0.007
. The transient was identified in deep James Webb Space Telescope (JWST)/NIRCam imaging from the JWST Advanced Deep Extragalactic Survey (JADES) program. Photometric and spectroscopic followup with NIRCam and NIRSpec, respectively, confirm the redshift and yield UV-NIR light-curve, NIR color, and spectroscopic information all consistent with a Type Ia classification. Despite its classification as a likely SN Ia, SN 2023adsy is both fairly red (
�
(
�
−
�
)
∼
0.9
) despite a host galaxy with low-extinction and has a high Ca II velocity (
19
,
000
±
2
,
000
km/s) compared to the general population of SNe Ia. While these characteristics are consistent with some Ca-rich SNe Ia, particularly SN 2016hnk, SN 2023adsy is intrinsically brighter than the low-
�
Ca-rich population. Although such an object is too red for any low-
�
cosmological sample, we apply a fiducial standardization approach to SN 2023adsy and find that the SN 2023adsy luminosity distance measurement is in excellent agreement (
≲
1
�
) with
Λ
CDM. Therefore unlike low-
�
Ca-rich SNe Ia, SN 2023adsy is standardizable and gives no indication that SN Ia standardized luminosities change significantly with redshift. A larger sample of distant SNe Ia is required to determine if SN Ia population characteristics at high-
�
truly diverge from their low-
�
counterparts, and to confirm that standardized luminosities nevertheless remain constant with redshift.
Signatures of wave erosion in Titan’s coastsSérgio Sacani
The shorelines of Titan’s hydrocarbon seas trace flooded erosional landforms such as river valleys; however, it isunclear whether coastal erosion has subsequently altered these shorelines. Spacecraft observations and theo-retical models suggest that wind may cause waves to form on Titan’s seas, potentially driving coastal erosion,but the observational evidence of waves is indirect, and the processes affecting shoreline evolution on Titanremain unknown. No widely accepted framework exists for using shoreline morphology to quantitatively dis-cern coastal erosion mechanisms, even on Earth, where the dominant mechanisms are known. We combinelandscape evolution models with measurements of shoreline shape on Earth to characterize how differentcoastal erosion mechanisms affect shoreline morphology. Applying this framework to Titan, we find that theshorelines of Titan’s seas are most consistent with flooded landscapes that subsequently have been eroded bywaves, rather than a uniform erosional process or no coastal erosion, particularly if wave growth saturates atfetch lengths of tens of kilometers.
SDSS1335+0728: The awakening of a ∼ 106M⊙ black hole⋆Sérgio Sacani
Context. The early-type galaxy SDSS J133519.91+072807.4 (hereafter SDSS1335+0728), which had exhibited no prior optical variations during the preceding two decades, began showing significant nuclear variability in the Zwicky Transient Facility (ZTF) alert stream from December 2019 (as ZTF19acnskyy). This variability behaviour, coupled with the host-galaxy properties, suggests that SDSS1335+0728 hosts a ∼ 106M⊙ black hole (BH) that is currently in the process of ‘turning on’. Aims. We present a multi-wavelength photometric analysis and spectroscopic follow-up performed with the aim of better understanding the origin of the nuclear variations detected in SDSS1335+0728. Methods. We used archival photometry (from WISE, 2MASS, SDSS, GALEX, eROSITA) and spectroscopic data (from SDSS and LAMOST) to study the state of SDSS1335+0728 prior to December 2019, and new observations from Swift, SOAR/Goodman, VLT/X-shooter, and Keck/LRIS taken after its turn-on to characterise its current state. We analysed the variability of SDSS1335+0728 in the X-ray/UV/optical/mid-infrared range, modelled its spectral energy distribution prior to and after December 2019, and studied the evolution of its UV/optical spectra. Results. From our multi-wavelength photometric analysis, we find that: (a) since 2021, the UV flux (from Swift/UVOT observations) is four times brighter than the flux reported by GALEX in 2004; (b) since June 2022, the mid-infrared flux has risen more than two times, and the W1−W2 WISE colour has become redder; and (c) since February 2024, the source has begun showing X-ray emission. From our spectroscopic follow-up, we see that (i) the narrow emission line ratios are now consistent with a more energetic ionising continuum; (ii) broad emission lines are not detected; and (iii) the [OIII] line increased its flux ∼ 3.6 years after the first ZTF alert, which implies a relatively compact narrow-line-emitting region. Conclusions. We conclude that the variations observed in SDSS1335+0728 could be either explained by a ∼ 106M⊙ AGN that is just turning on or by an exotic tidal disruption event (TDE). If the former is true, SDSS1335+0728 is one of the strongest cases of an AGNobserved in the process of activating. If the latter were found to be the case, it would correspond to the longest and faintest TDE ever observed (or another class of still unknown nuclear transient). Future observations of SDSS1335+0728 are crucial to further understand its behaviour. Key words. galaxies: active– accretion, accretion discs– galaxies: individual: SDSS J133519.91+072807.4
Order : Trombidiformes (Acarina) Class : Arachnida
Mites normally feed on the undersurface of the leaves but the symptoms are more easily seen on the uppersurface.
Tetranychids produce blotching (Spots) on the leaf-surface.
Tarsonemids and Eriophyids produce distortion (twist), puckering (Folds) or stunting (Short) of leaves.
Eriophyids produce distinct galls or blisters (fluid-filled sac in the outer layer)
BIRDS DIVERSITY OF SOOTEA BISWANATH ASSAM.ppt.pptxgoluk9330
Ahota Beel, nestled in Sootea Biswanath Assam , is celebrated for its extraordinary diversity of bird species. This wetland sanctuary supports a myriad of avian residents and migrants alike. Visitors can admire the elegant flights of migratory species such as the Northern Pintail and Eurasian Wigeon, alongside resident birds including the Asian Openbill and Pheasant-tailed Jacana. With its tranquil scenery and varied habitats, Ahota Beel offers a perfect haven for birdwatchers to appreciate and study the vibrant birdlife that thrives in this natural refuge.
Compositions of iron-meteorite parent bodies constrainthe structure of the pr...Sérgio Sacani
Magmatic iron-meteorite parent bodies are the earliest planetesimals in the Solar System,and they preserve information about conditions and planet-forming processes in thesolar nebula. In this study, we include comprehensive elemental compositions andfractional-crystallization modeling for iron meteorites from the cores of five differenti-ated asteroids from the inner Solar System. Together with previous results of metalliccores from the outer Solar System, we conclude that asteroidal cores from the outerSolar System have smaller sizes, elevated siderophile-element abundances, and simplercrystallization processes than those from the inner Solar System. These differences arerelated to the formation locations of the parent asteroids because the solar protoplane-tary disk varied in redox conditions, elemental distributions, and dynamics at differentheliocentric distances. Using highly siderophile-element data from iron meteorites, wereconstruct the distribution of calcium-aluminum-rich inclusions (CAIs) across theprotoplanetary disk within the first million years of Solar-System history. CAIs, the firstsolids to condense in the Solar System, formed close to the Sun. They were, however,concentrated within the outer disk and depleted within the inner disk. Future modelsof the structure and evolution of the protoplanetary disk should account for this dis-tribution pattern of CAIs.
Sexuality - Issues, Attitude and Behaviour - Applied Social Psychology - Psyc...PsychoTech Services
A proprietary approach developed by bringing together the best of learning theories from Psychology, design principles from the world of visualization, and pedagogical methods from over a decade of training experience, that enables you to: Learn better, faster!
Evidence of Jet Activity from the Secondary Black Hole in the OJ 287 Binary S...Sérgio Sacani
Wereport the study of a huge optical intraday flare on 2021 November 12 at 2 a.m. UT in the blazar OJ287. In the binary black hole model, it is associated with an impact of the secondary black hole on the accretion disk of the primary. Our multifrequency observing campaign was set up to search for such a signature of the impact based on a prediction made 8 yr earlier. The first I-band results of the flare have already been reported by Kishore et al. (2024). Here we combine these data with our monitoring in the R-band. There is a big change in the R–I spectral index by 1.0 ±0.1 between the normal background and the flare, suggesting a new component of radiation. The polarization variation during the rise of the flare suggests the same. The limits on the source size place it most reasonably in the jet of the secondary BH. We then ask why we have not seen this phenomenon before. We show that OJ287 was never before observed with sufficient sensitivity on the night when the flare should have happened according to the binary model. We also study the probability that this flare is just an oversized example of intraday variability using the Krakow data set of intense monitoring between 2015 and 2023. We find that the occurrence of a flare of this size and rapidity is unlikely. In machine-readable Tables 1 and 2, we give the full orbit-linked historical light curve of OJ287 as well as the dense monitoring sample of Krakow.
Embracing Deep Variability For Reproducibility and Replicability
Abstract: Reproducibility (aka determinism in some cases) constitutes a fundamental aspect in various fields of computer science, such as floating-point computations in numerical analysis and simulation, concurrency models in parallelism, reproducible builds for third parties integration and packaging, and containerization for execution environments. These concepts, while pervasive across diverse concerns, often exhibit intricate inter-dependencies, making it challenging to achieve a comprehensive understanding. In this short and vision paper we delve into the application of software engineering techniques, specifically variability management, to systematically identify and explicit points of variability that may give rise to reproducibility issues (eg language, libraries, compiler, virtual machine, OS, environment variables, etc). The primary objectives are: i) gaining insights into the variability layers and their possible interactions, ii) capturing and documenting configurations for the sake of reproducibility, and iii) exploring diverse configurations to replicate, and hence validate and ensure the robustness of results. By adopting these methodologies, we aim to address the complexities associated with reproducibility and replicability in modern software systems and environments, facilitating a more comprehensive and nuanced perspective on these critical aspects.
https://hal.science/hal-04582287
Microbial interaction
Microorganisms interacts with each other and can be physically associated with another organisms in a variety of ways.
One organism can be located on the surface of another organism as an ectobiont or located within another organism as endobiont.
Microbial interaction may be positive such as mutualism, proto-cooperation, commensalism or may be negative such as parasitism, predation or competition
Types of microbial interaction
Positive interaction: mutualism, proto-cooperation, commensalism
Negative interaction: Ammensalism (antagonism), parasitism, predation, competition
I. Mutualism:
It is defined as the relationship in which each organism in interaction gets benefits from association. It is an obligatory relationship in which mutualist and host are metabolically dependent on each other.
Mutualistic relationship is very specific where one member of association cannot be replaced by another species.
Mutualism require close physical contact between interacting organisms.
Relationship of mutualism allows organisms to exist in habitat that could not occupied by either species alone.
Mutualistic relationship between organisms allows them to act as a single organism.
Examples of mutualism:
i. Lichens:
Lichens are excellent example of mutualism.
They are the association of specific fungi and certain genus of algae. In lichen, fungal partner is called mycobiont and algal partner is called
II. Syntrophism:
It is an association in which the growth of one organism either depends on or improved by the substrate provided by another organism.
In syntrophism both organism in association gets benefits.
Compound A
Utilized by population 1
Compound B
Utilized by population 2
Compound C
utilized by both Population 1+2
Products
In this theoretical example of syntrophism, population 1 is able to utilize and metabolize compound A, forming compound B but cannot metabolize beyond compound B without co-operation of population 2. Population 2is unable to utilize compound A but it can metabolize compound B forming compound C. Then both population 1 and 2 are able to carry out metabolic reaction which leads to formation of end product that neither population could produce alone.
Examples of syntrophism:
i. Methanogenic ecosystem in sludge digester
Methane produced by methanogenic bacteria depends upon interspecies hydrogen transfer by other fermentative bacteria.
Anaerobic fermentative bacteria generate CO2 and H2 utilizing carbohydrates which is then utilized by methanogenic bacteria (Methanobacter) to produce methane.
ii. Lactobacillus arobinosus and Enterococcus faecalis:
In the minimal media, Lactobacillus arobinosus and Enterococcus faecalis are able to grow together but not alone.
The synergistic relationship between E. faecalis and L. arobinosus occurs in which E. faecalis require folic acid
MICROBIAL INTERACTION PPT/ MICROBIAL INTERACTION AND THEIR TYPES // PLANT MIC...
Nuclear Reaction Taking Different Weight Target Nucleus
1. International Journal of Recent Advances in Physics (IJRAP) Vol.6, No.1, February 2017
DOI : 10.14810/ijrap.2017.6101 1
NUCLEAR REACTION TAKING DIFFERENT WEIGHT
TARGET NUCLEUS
Rohit Gupta
Department of Physics, Institute of Basic Sciences, Dr. Bhim Rao Ambedkar University,
Khandari Campus, Agra (U.P.)-India.
ABSTRACT
The nuclear reactions are very interesting and very big topic in research field, In this research paper we
are describing about all types of nuclear reactions taking for light weight, medium weight and heavy
weight target nucleus, which is only one types of target nucleus.
Here our interest how many types nuclear reactions occur or don't occur at taking for light weight, medium
weight and heavy weight target nucleus. Finding the reason why it doesn't become to taking other weight
target nucleus and why it becomes in those types of targets nucleus. So we can say it can become very
interesting topic in field of finding new information about nucleus reactions to taking different types of
targets nucleus.
KEYWORDS
Higgs boson, nuclear fission, nuclear fusion, incident particle, nuclear reaction and elementary particles.
1. INTRODUCTION
Here our interest taking only one nucleus which is in the form of light nucleus, medium nucleus
and heavy nucleus in rest position and changed in the incident particles and its kinetic energy, we
can mostly perform all types of nuclear reactions. But some nuclear reactions don't perform in
light nucleus, medium nucleus and heavy nucleus, so we see here whose nuclear reactions don't
perform in light nucleus, medium nucleus and heavy nucleus and why, getting its proper reason.
Here we kwon that the light nucleus (A < 40) mass number equal to or less than 40, medium
nucleus (40 < A < 150) mass number less than 150 and heavy nucleus (A > 150) the mass number
large than 200.
So here we take any light nucleus under 40, medium nucleus under 150 and heavy nucleus more
than 150.
2. NUCLEAR REACTIONS
In the nuclear reactions target nucleus and incident particle approach to each other, there are
mainly some types of nuclear reactions also perform.
2.1. ELASTIC REACTION
When the incident particle don't enter field of targets nucleus it means don't changes inside
nucleus and the target nucleus same as, this types of reactions isn't nuclear reactions, it's simply
Elastic Reaction[2].
4
He2 + 197
Au79 → 197
Au79+ 4
He2
2. International Journal of Recent Advances in Physics (IJRAP) Vol.6, No.1, February 2017
2
2.2. INELASTIC REACTION
When the incident particles entre inside the field of target nucleus, incident particle loss energy
on target nucleus and target nucleus reached in exited state, after loss exited energy the target
nucleus come on ground state. It’s called Inelastic Reaction [2].
7
Li3 + 1
H1 → (7
Li3)* + 1
H1
2.3. COMPOUND NUCLEAR REACTION
When the incident particle break potential barrier of the target nucleus, the target nucleus and
incident particle combined for very low time period also remains for a long time (≅10-16
sec)
compared to small time (≅10-22
sec) and it is in highly exited state. Its called compound nuclear
reactions.
There are many types of compound nuclear reactions basis of product nucleus and eject
particle[1].
2.3.1. Disintegration
The incident particle strikes on the target nuclei, absorbed by it and a different particle is ejected
by it, the product nucleus also different from target nucleus.
14
N7 + 4
He2 → (18
F9)* → 17
O8 + 1
H1
2.3.2. Photo Disintegration
The γ-ray particle also absorbed by the target nucleus, after absorbed γ- ray the target nucleus
reached in excited higher quantum state. If the energy is high enough, one or more particles may
be reduce form it [1].
2
H1 + γ → (2
H1)* → 1
H1 + 1
n0
2.3.3. Radioactive Capture
When the incident particle break potential barrier of the target nucleus, the target nucleus and
incident particle combined and product nucleus low exited state than only γ photon is reduce by
it.
26
Mg12 + 1
H1 → (27
Al13)* → 27
Al13 + γ
2.4. DIRECT REACTIONS
Incident particle collides with target nucleus. In this process compound nucleus don't make and
reaction performs very low time less than 10-22 sec. There are two types of Direct Reactions.
2.4.1. Pickup Reaction
In this type of reaction, the incident particle loses one or more nucleons on the target nucleus.
63
Cu29 + 2
H1 → 64
Cu29 + 1
H1
2.4.2. Stripping Reaction
In this types of reaction, the target nucleus loss one or more particles at incident particle[5].
3. International Journal of Recent Advances in Physics (IJRAP) Vol.6, No.1, February 2017
3
7
Li3 + 1
H1 → 6
Li3 + 2
H1
2.5. SPONTANEOUS DECAY
The spontaneous reactions don't under control, in this Alfa and Beta particle decay form nucleus.
7
Li3 → 7
Be4 + 0
β-1 + ν
2.6. SPALLATION REACTIONS
The incident particle capture by a heavy target nucleus, several particles of sufficient energy
ejected from it, It is also known Spallation Reaction. The nuclear fission is a good example it.
235
U92 + 1
n0 → 98
Zr40 + 136
Te52 + 21
n0
2.7. HIGH ENERGY REACTIONS
In High Energy Reaction the energy range of incident particle about 150 MeV, the new kinds of
particles (mesons, strange particles) are ejected from nucleons[1].
2.8. HEAVY ION REACTIONS
The nuclear reactions inducted by heavy ions (A≥12), the reaction mechanism, such as coulomb
excitation, elastic scattering, direct reactions and compound nucleus.
The nuclear reactions also process on the basis of incident practical, its energy and target nucleus
such as[1].
2.8.1. Transfer Reaction (Direct Reaction)
14
N7 + 10
B5 → 13
N7 + 11
B5
2.8.2. Neutron Reactions
93
Nb41 + 12
C6 → 103
Ag47 + 21
n0
2.8.3. Fission Spallation And Fragmentation Reaction
27
Al13 + 14
N7 → (41
Ca20)* → 1
H1 + 21
n0 + 38
K19
3. NUCLEAR REACTIONS ON THE BASIS OF WEIGHT OF TARGET NUCLEUS
There we are using light weight target nucleus, medium weight target nucleus and heavy weight
target nucleus.
3.1. Light Weight Target Nucleus
Let here we can take 7Li3 for target nucleus in nuclear reactions and nuclear reactions are
perform as following.
3.1.1. Elastic Reaction
In light weight target nucleus, elastic reaction is possible.
7
Li3 + 4
He2 → 7
Li3 + 4
He2
4. International Journal of Recent Advances in Physics (IJRAP) Vol.6, No.1, February 2017
4
3.1.2. Inelastic Reaction
In light weight target nucleus, inelastic reaction is possible.
7
Li3 + 4
He2 → (7
Li3)* + 4
He2
3.1.3. Compound Nuclear Reaction
In light weight target nucleus, all types compound nuclear reaction are possible.
3.1.3.1. Disintegration
7
Li3 + 4
He2 → (11
Be5)* → 10
B5 + 1
n
3.1.3.2. Photo Disintegration
7
Li3 + γ → (7
Li3)* → 4
He2 + 3
H1
3.1.3.3. Radioactive Capture
7
Li3 + 4
He2 → (11
Be5)* → 11
Be5 + γ
3.1.4. Direct Reactions
In light weight target nucleus, both types direct reaction are possible.
3.1.4.1. Pickup Reaction
7
Li3 + 2
H1 → 8
Li3 + 1
H1
3.1.4.2. Stripping Reaction
7
Li3 + 1
H1 → 6
Li3 + 2
H1
3.1.5. Spontaneous Decay
In light weight target nucleus, spontaneous decay is possible.
11
Li3 → 11
Be4 + 0
β-1 + ν
3.1.5. Spallation Reaction
The spallation reaction is not possible in light weight target nucleus, it become only heavy weight
target nucleus.
3.1.6. High Energy Reactions
It is possible taking light weight target nucleus. In it, the particles (meson, strange particles)
produce by nucleons (proton, neutron).
3.1.7. Heavy Ion Reactions
It is not possible taking light weight target nucleus.
5. International Journal of Recent Advances in Physics (IJRAP) Vol.6, No.1, February 2017
5
3.1.7.1. Transfer Reaction (Direct Reaction)
7
Li3 + 6
Li3 → 9
Be4 + 4
He2
3.1.7.2. Neutron Reaction
7
Li3 + 7
Li3 → 12
C6 + 21
n0
3.1.7.3. Fission Spallation And Fragmentation Reaction
27
Al13 + 14
N7 → (41
Ca20)* → 38
K19 + 1
H1 + 21
n0
3.2. Medium Weight Target Nucleus
Let here we can take Cu for target nucleus in nuclear reactions and nuclear reactions are perform
as following.
3.2.1. Elastic Reaction
Elastic reaction is possible taking medium weight target nucleus.
65
Cu29 + 4
He2 → 65
Cu29 + 4
He2
3.2.2. Inelastic Reaction
Inelastic reaction is possible talking medium weight target nucleus.
65
Cu29 + 4
He2 → (65
Cu29)* + 4
He2
3.2.3. Compound Nuclear Reaction
In medium weight target nucleus, all types compound nuclear reaction are possible.
3.2.3.1. Disintegration
65
Cu29 + 1H1 → (66
Zn30)* → 65
Zn30 + 1
n0
3.2.3.2. Photo Disintegration
65
Cu29 + γ → (65
Cu29)* → 65
Cu29 + γ′
3.2.3.3. Radioactive Capture
65
Cu29 + 0
n1 → (66
Cu29)* → 66
Cu29 + γ
3.2.4. Direct Reactions
In medium weight target nucleus, both type direct reactions are possible.
3.2.4.1. Pickup Reaction
63
Cu29 + 2
H1 → 64
Cu29 + 1
H1
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3.2.4.2. Stripping Reaction
64
Cu29 + 1
H1 → 63
Cu29 + 2
H1
3.2.5. Spontaneous Decay
In medium weight target nucleus, spontaneous decay is also possible.
64
Cu29 → 64
Zn30 + 0
β-1 + ν
3.2.6. Spallation Reaction
The spallation reaction is not possible in medium weight target nucleus, it become only heavy
weight target nucleus.
3.2.7. High Energy Reactions
It is possible taking medium weight target nucleus. In it, the particles (meson, strange particles)
produce by nucleons (proton, neutron).
3.2.8. Heavy Ion Reactions
In medium weight target nucleus, several heavy ion reaction possible and several not possible.
As transfer reaction (direct reaction) and neutron reaction is also possible but fission spallation
and fragmentation reaction is not possible[8].
3.2.8.1. Transfer Reaction (Direct Reaction)
65
Cu29 + 13
N7 → 63
Cu29 + 15
N7 → (65
Zn30 + 13
C6)
3.2.8.2. Neutron Reactions
65
Cu29 + 14
N7 → 78
Kr36 + 1
n0
3.2.8. 3. Fission Spallation And Fragmentation Reaction
It is no possible in medium weight target nucleus.
3.3. HEAVY WEIGHT TARGET NUCLEUS
Let here we can take Au for target nucleus in nuclear reactions and nuclear reactions are perform
as following[8].
3.3.1. Elastic Reaction
Taking heavy weight target nucleus, elastic reaction is possible.
197
Au79 +4
He2 → 197
Au79 + 4
He2
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3.3.2 Inelastic Reaction
Taking heavy weight target nucleus, inelastic reaction is possible.
3.3.3. Compound Nuclear Reaction
Taking heavy weight target nucleus, all types compound nuclear reaction is possible.
3.3.3.1. Disintegration
197
Au79 + 3
H1 → (200
Hg80)* → 199
Hg80 + 1
n0
3.3.3.2. Photo Disintegration
197
Au79 + γ → (197
Au79)* → 197
Au79 + γ′
3.3.3.3 Radioactive Capture
197
Au79 + 1
n0 → (198
Au79)* → 198
Au79 + y
3.3.4. Direct Reactions
Taking heavy weight target nucleus, all type direct reaction is possible.
3.3.4.1. Pickup Reaction
197
Au79 + 2
H1 → 198
Au79 + 1
H1
3.3.4.2. Stripping Reaction
197
Au79 + 1
H1 → 196
Au79 + 2
H1
3.3.5. Spontaneous Decay
Taking heavy weight target nucleus, spontaneous reaction is possible.
198
Au79 → 198
Hg80 + 0
β-1 + ν
3.3.6. Spallation Reaction
It is possible in some heavy weight target nucleus, but not for all, it is not possible in Au target
nucleus.
The suitable example is
235
U92 + 1
n0 → (136
U92)* → 92
Kr36 + 141
Ba56 + 31
n0 + γ(energy)
3.3.7. High Energy Reactions
It is possible taking heavy weight target nucleus. In it the particles (meson, strange particle)
produce by nucleons (proton and neutron).
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3.3.8. Heavy Ion Reactions
In heavy weight target nucleus, several nuclear reactions are possible and several rarely possible
like, transfer reaction (direct reaction) and neutron reaction is also possible but fission spallation
and fragmentation reaction is rarely possible[9].
3.3.8.1. Transfer Reaction (Direct Reaction)
197
Au79 + 14
N7 → 196
Pt78 + 15
O8
3.3.8.2. Neutron Reactions
197
Au79 + 12
C6 → 205
At85 + 41
n0
3.3.8.3. Fission Spallation And Fragmentation Reaction
235
U92 + 1
n0 → (236
U92)* → 98
Zr40 + 136
Te52 + 21
n0
4. THE RESULT
In this, nuclear reaction (light weight, medium weight and heavy weight target) several types
nuclear reactions become or don't become. The name of nuclear reactions which don't become
each one as spallation reactions, High energy, Heavy ions reaction, Fission, etc. and the any other
nuclear reactions become each one.
Any nuclear fusion possible in light weight nucleus (A>20), Nuclear fission rarely possible in
medium weight nucleus and large possibility in heavy weight nucleus.
5. CONCLUSION
The several types of nuclear reaction which don't become or become taking weight target nucleus.
We can understand that type nuclear reaction and classified it, in two ways as, target nucleus
dependent nuclear reactions and nondependent nuclear reactions. It is very useful phenomena in
nuclear transmutation. This type we can take any target nucleus and see by nuclear reaction or
table nuclear transmutation must do.
REFERENCES
[1] Nuclear Physics book D.C. Tayal (Himalaya Publishing House) ISO 9001:2008 Certified.
[2] Burhan, W.E."Nuclear Physics", McGraw Hill Co. New York.
[3] Roy R.R. And B.P. Nigam,"Nuclear Physics", John Wiley, New York, 1967.
[4] Enge, Harald A. "Introduction to Nuclear Physics", Addition -Wesley,1966.
[5] butler, S.T., “Nuclear Stripping Reaction”, John Wiley, New York, 1957.
[6] Condon E.U. and Hugh Odishaw, “Hand-book of Physics”, McGraw Hill, 1967.
[7] Prashant Kumar,IEC College of Engineering and Technology, India.“Nano Nuclear Reaction”,
International Journal of Emerging Research and Technology.
[8] MasreshaFeleke, “Some Basics of Nuclear Reactions”, ADDIS ABABA UNIVERSITY, ADDIS
ABABA, ETHIOPIA (June 2011).
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[9] Ankit Gupta and Rustum Sengupta, DEI Dayalbagh Agra- 282005. “Analytical Study of Department
of NuclearFusion Reactors As Potential Source of Energy in the Future”.
[10] Steven B. Krivit and Jan Marwan, “A New Look at Low-Energy Nuclear Reaction Research” (Sep-
2009), Journal of Environmental Monitoring.
[11] Hans Henrik Knudsen, Department of Physics and Astronomy University of Aarhus, “ Low
Energy Nuclear Reaction, Exploratory Work on11B” (August-2008), Sodium Petit in Profundis,
UniversitasArhusiensis.
AUTHOR
Rohit Gupta is a M.Sc. form Agra, College Agra from Physics. Rohit Gupta is in
Department of Physics, Institute of basic Sciences, Dr. Bhim Rao Ambedkar University,
Khandari Campus, Agra (U.P.)-India