The document discusses radioactive decay and nuclear fission. It explains that the half-life of an isotope is the time it takes for half of its atoms to decay. It provides examples of isotopes like radium-226 and discusses where they come from. The strong nuclear force holds atomic nuclei together, and some heavy nuclei are radioactive because they can reach a lower potential energy state through decay. Nuclear fission occurs when an unstable nucleus splits into smaller nuclei, often emitting free neutrons which can then trigger further fissions in a chain reaction.
Intriguing Neutrinos: The Deep Secrets of Nature’s Ghosts by Dr Elisabeth Falkonthewight
Lisa Falk's presentation about the Neutrino, one of the fundamental particles which make up the universe - Also, currently, one of the least understood.
Subatomic particles produced by the decay of radioactive elements. They're special for many reasons - They have no charge, are incredibly light, travel at near light speed and travel through most other matter.
Following the introduction to what they are, she detailed the challenges of detecting them (she's been directly involved in these experiments, including time at CERN), and the vast equipment that's used.
Finally she talked about the DUNE project, the next stage in Neutrino detection.
Presented to Cafe Scientifique, Isle of Wight, 11th May 2015.
The ninth science topic in our survey of groundbreaking New Energy sciences that allow us to extract clean, limitless energy from the quantum vacuum. This topic is Low-Energy Nuclear Reactions, also known by the name Cold Fusion.
Besides the 4 fundamental forces established and accepted by current science community, a new force is to be added. This is the familiar mechanical force mediated by the particle 'Phonon'. A new discovery.
Intriguing Neutrinos: The Deep Secrets of Nature’s Ghosts by Dr Elisabeth Falkonthewight
Lisa Falk's presentation about the Neutrino, one of the fundamental particles which make up the universe - Also, currently, one of the least understood.
Subatomic particles produced by the decay of radioactive elements. They're special for many reasons - They have no charge, are incredibly light, travel at near light speed and travel through most other matter.
Following the introduction to what they are, she detailed the challenges of detecting them (she's been directly involved in these experiments, including time at CERN), and the vast equipment that's used.
Finally she talked about the DUNE project, the next stage in Neutrino detection.
Presented to Cafe Scientifique, Isle of Wight, 11th May 2015.
The ninth science topic in our survey of groundbreaking New Energy sciences that allow us to extract clean, limitless energy from the quantum vacuum. This topic is Low-Energy Nuclear Reactions, also known by the name Cold Fusion.
Besides the 4 fundamental forces established and accepted by current science community, a new force is to be added. This is the familiar mechanical force mediated by the particle 'Phonon'. A new discovery.
The eleventh part in our survey of emerging New Energy sciences. This is possibly one of New Energy's most promising fields - that of quantum heat engines. Quantum ratchets or heat engines may one day be used to power our mobile devices without ever needing to be charged. They may also power nanobots inside our bodies for targeted delivery of medicines, arterial cleansing, etc.
Lattice Energy LLC - Many body collective magnetic mechanism creates ultrahig...Lewis Larsen
“The main reason why the origin of cosmic rays(CRs) is still unknown, one century after their discovery, is that they are charged nuclei isotropized by the turbulent magnetic field in the Galaxy to such a high degree that their observed flux is essentially identical in all directions, with no sources or decisive hot spots identified in any region the sky …” - Etienne Parizot (Univ. of Paris-Diderot), Nuclear Physics B (2014)
In 2008 (arXiv) and 2010 (Pramana), we derived and published approximate, rule-of-thumb formulas for calculating estimated one-shot, mean center-of-mass acceleration energies for charged particles present in plasma-filled magnetic flux tubes (also called “coronal loops”) for two cases: (1) steady-state and (2) explosive destruction of an unstable flux tube (this second case is subset of “magnetic reconnection” processes).
Our simple equations for magnetic flux tubes are robust and scale-independent. They consequently have broad applicability from exploding wires (which in early stages of explosion comprise dense dusty plasmas), lightning, to solar flux tubes and other astrophysical environments that are characterized by vastly higher magnetic fields; these include many other types of stars besides the Sun, neutron stars, magnetars, and regions located near black holes and active galactic nuclei.
Herein we show how plasma-filled magnetic flux tubes likely occur in many different astrophysical systems from relatively small objects (neutron stars and magnetars) to relatively large objects (accretion disks and jet bases of supermassive black holes). When these ordered magnetic structures explode (reconnection, flares), enormous amounts of magnetic energy are converted into kinetic energy of charged particles present inside exploding flux tubes. Using reasonable parametric assumptions, we calculate one-shot, center-of-mass acceleration energies for protons in collapsing protoneutron stars (5.5 x 1018 eV), two cases for BH accretion disks (2.2 x 1017 eV and 0.9 x 1019 eV), and finally for the jet base of a supermassive black hole (2.2 x 1021eV).
What all these numbers suggest, including those for the Sun, is that W-L-S particle acceleration mechanism for magnetic flux tubes can create cosmic ray particles at energies that span the entire cosmic-ray energy spectrum from top to bottom. This argues that commonplace flux tubes may well play a significant role in generating the observed cosmic ray energy spectrum and would be consistent with apparent overall anisotropy of sources at all but the very highest particle energies. That said, we think a number of different acceleration mechanisms likely contribute to entire spectrum, including shock acceleration and perhaps exotic mechanisms such as evaporation of gaseous winds from neutron stars (Widom et al. arXiv:1410.6498v2 -2015).
The Large Hadron Collider (LHC) is the world's largest and most powerful particle collider, most complex experimental facility ever built, and the largest single machine in the world.
It was built by the European Organization for Nuclear Research (CERN) between 1998 and 2008 in collaboration with over 10,000 scientists and engineers from over 100 countries, as well as hundreds of universities and laboratories.
The Higgs boson is an elementary particle in the Standard Model of particle physics. It is the quantum excitation of the Higgs field, a fundamental field of crucial importance to particle physics theory first suspected to exist in the 1960s and was discovered in 2012 in lhc.
Inside the accelerator, two high-energy particle beams travel at close to the speed of light before they are made to collide. The beams travel in opposite directions in separate beam pipes – two tubes kept at ultrahigh vacuum. They are guided around the accelerator ring by a strong magnetic field maintained by superconducting electromagnets.
The God Particle or God particle may refer to: Higgs boson, a particle in physics sometimes referred to as the God's Particle.
The fourth area of modern science we consider fundamental to understanding and applying New Energy -- also called Zero Point Energy. This is the field of Quantum Electrodynamics.
The eleventh part in our survey of emerging New Energy sciences. This is possibly one of New Energy's most promising fields - that of quantum heat engines. Quantum ratchets or heat engines may one day be used to power our mobile devices without ever needing to be charged. They may also power nanobots inside our bodies for targeted delivery of medicines, arterial cleansing, etc.
Lattice Energy LLC - Many body collective magnetic mechanism creates ultrahig...Lewis Larsen
“The main reason why the origin of cosmic rays(CRs) is still unknown, one century after their discovery, is that they are charged nuclei isotropized by the turbulent magnetic field in the Galaxy to such a high degree that their observed flux is essentially identical in all directions, with no sources or decisive hot spots identified in any region the sky …” - Etienne Parizot (Univ. of Paris-Diderot), Nuclear Physics B (2014)
In 2008 (arXiv) and 2010 (Pramana), we derived and published approximate, rule-of-thumb formulas for calculating estimated one-shot, mean center-of-mass acceleration energies for charged particles present in plasma-filled magnetic flux tubes (also called “coronal loops”) for two cases: (1) steady-state and (2) explosive destruction of an unstable flux tube (this second case is subset of “magnetic reconnection” processes).
Our simple equations for magnetic flux tubes are robust and scale-independent. They consequently have broad applicability from exploding wires (which in early stages of explosion comprise dense dusty plasmas), lightning, to solar flux tubes and other astrophysical environments that are characterized by vastly higher magnetic fields; these include many other types of stars besides the Sun, neutron stars, magnetars, and regions located near black holes and active galactic nuclei.
Herein we show how plasma-filled magnetic flux tubes likely occur in many different astrophysical systems from relatively small objects (neutron stars and magnetars) to relatively large objects (accretion disks and jet bases of supermassive black holes). When these ordered magnetic structures explode (reconnection, flares), enormous amounts of magnetic energy are converted into kinetic energy of charged particles present inside exploding flux tubes. Using reasonable parametric assumptions, we calculate one-shot, center-of-mass acceleration energies for protons in collapsing protoneutron stars (5.5 x 1018 eV), two cases for BH accretion disks (2.2 x 1017 eV and 0.9 x 1019 eV), and finally for the jet base of a supermassive black hole (2.2 x 1021eV).
What all these numbers suggest, including those for the Sun, is that W-L-S particle acceleration mechanism for magnetic flux tubes can create cosmic ray particles at energies that span the entire cosmic-ray energy spectrum from top to bottom. This argues that commonplace flux tubes may well play a significant role in generating the observed cosmic ray energy spectrum and would be consistent with apparent overall anisotropy of sources at all but the very highest particle energies. That said, we think a number of different acceleration mechanisms likely contribute to entire spectrum, including shock acceleration and perhaps exotic mechanisms such as evaporation of gaseous winds from neutron stars (Widom et al. arXiv:1410.6498v2 -2015).
The Large Hadron Collider (LHC) is the world's largest and most powerful particle collider, most complex experimental facility ever built, and the largest single machine in the world.
It was built by the European Organization for Nuclear Research (CERN) between 1998 and 2008 in collaboration with over 10,000 scientists and engineers from over 100 countries, as well as hundreds of universities and laboratories.
The Higgs boson is an elementary particle in the Standard Model of particle physics. It is the quantum excitation of the Higgs field, a fundamental field of crucial importance to particle physics theory first suspected to exist in the 1960s and was discovered in 2012 in lhc.
Inside the accelerator, two high-energy particle beams travel at close to the speed of light before they are made to collide. The beams travel in opposite directions in separate beam pipes – two tubes kept at ultrahigh vacuum. They are guided around the accelerator ring by a strong magnetic field maintained by superconducting electromagnets.
The God Particle or God particle may refer to: Higgs boson, a particle in physics sometimes referred to as the God's Particle.
The fourth area of modern science we consider fundamental to understanding and applying New Energy -- also called Zero Point Energy. This is the field of Quantum Electrodynamics.
Osmotic stress and water isotope effects in kinesin-1 gliding motility assaysSteve Koch
The osmotic pressure and kinetic properties of water play important roles in biomolecular interactions. As pointed out by Parsegian, Rand, and Rau, these crucial roles are often overlooked1. In some fields, osmotic stress and isotope effects have been exploited for probing the role water plays in binding interactions of biomolecules. To our knowledge, there have been no studies of osmotic stress and water isotope effects for kinesin, and only a handful for myosin. We’re currently using the gliding motility assay to see whether we can extract new information about kinesin-1 / microtubule interactions by changing osmotic stress and water isotopes. We will describe our open-source, automated analysis platform for extracting microtubule gliding speeds from image series. We will also show our preliminary analyses of the changes seen in gliding assays when done in heavy water (either heavy-hydrogen or heavy-oxygen) or osmolytes (betaine). We will discuss whether osmotic stress and isotopes, particularly heavy-oxygen water, might be an important tool for probing effects of water on binding interactions between kinesin and microtubules. We will also discuss potential applications of deuterium water for stabilizing microtubules and kinesin for lab or device applications.
[1] Parsegian, V. A., Rand, R. P., & Rau, D. C. (1995). Macromolecules and water: probing with osmotic stress. Methods in Enzymology, 259.
This work was supported by the DTRA CB Basic Research Program under Grant No. HDTRA1-09-1-008 in collaboration with Dr. Susan Atlas lab (UNM).
2011 NSF CAREER_Steve Koch Full Project Description Steve Koch
This is the full Project Description for my 2011 NSF CAREER proposal. As I described on my blog, I am disappointed in the unfinished product, mostly because I still think the proposed research is important, exciting, and achievable by my lab. ( http://stevekochresearch.blogspot.com/2011/08/2011-nsf-career-proposal-ugh-failures.html )
Here are links to prior years' proposals, which were declined:
* 2009 http://www.scribd.com/doc/17548381/2009-ProposalCAREER-SingleMolecule-Analysis-of-Genomic-DNA-and-Chromatin-in-Eukaryotic-Transcription
* 2008 http://www.scribd.com/doc/10196076/2008-NSF-CAREERproposal-Only
This is a summary I gave at group meeting today on what I'd learned about D2O (aka "heavy water" aka "deuterium oxide") and its effects on biochemistry/biophysics of enzymes and proteins.
2009 September Kinesin Talk at UNM ChemistrySteve Koch
Talk given by Steve at the Unviversity of New Mexico Chemistry Department on September 11, 2009. It is mostly still an introduction to our kinesin project, but now I'm able to include the latest results from gliding motility assay, tracking software, and stochastic kinetics simulation.
Here are the slides describing talents and hedgehog concepts in the context of students' future careers. It's the background to our final assignment for the semester: http://openwetware.org/wiki/User:Steven_J._Koch/Talents_assignment
Discussion of dispersion and rainbows. Also some cool photos of blackbody and fluorescent spectra from Tom Decaro and Analisa Goodman as part of the homework question.
08 Feb 17 Light, Electron E Levels Actual PresentedSteve Koch
Introduction to electromagnetic radiation and light. Viewing atomic spectra with diffraction gratings. Optical tweezers (cool example of light having momentum).
This is lecture 5, Wave interference, standing waves, resonance, intro to sound waves. For Conceptual Physics course, Physics 102, at University of New Mexico. Koch's section.
Read| The latest issue of The Challenger is here! We are thrilled to announce that our school paper has qualified for the NATIONAL SCHOOLS PRESS CONFERENCE (NSPC) 2024. Thank you for your unwavering support and trust. Dive into the stories that made us stand out!
The Roman Empire A Historical Colossus.pdfkaushalkr1407
The Roman Empire, a vast and enduring power, stands as one of history's most remarkable civilizations, leaving an indelible imprint on the world. It emerged from the Roman Republic, transitioning into an imperial powerhouse under the leadership of Augustus Caesar in 27 BCE. This transformation marked the beginning of an era defined by unprecedented territorial expansion, architectural marvels, and profound cultural influence.
The empire's roots lie in the city of Rome, founded, according to legend, by Romulus in 753 BCE. Over centuries, Rome evolved from a small settlement to a formidable republic, characterized by a complex political system with elected officials and checks on power. However, internal strife, class conflicts, and military ambitions paved the way for the end of the Republic. Julius Caesar’s dictatorship and subsequent assassination in 44 BCE created a power vacuum, leading to a civil war. Octavian, later Augustus, emerged victorious, heralding the Roman Empire’s birth.
Under Augustus, the empire experienced the Pax Romana, a 200-year period of relative peace and stability. Augustus reformed the military, established efficient administrative systems, and initiated grand construction projects. The empire's borders expanded, encompassing territories from Britain to Egypt and from Spain to the Euphrates. Roman legions, renowned for their discipline and engineering prowess, secured and maintained these vast territories, building roads, fortifications, and cities that facilitated control and integration.
The Roman Empire’s society was hierarchical, with a rigid class system. At the top were the patricians, wealthy elites who held significant political power. Below them were the plebeians, free citizens with limited political influence, and the vast numbers of slaves who formed the backbone of the economy. The family unit was central, governed by the paterfamilias, the male head who held absolute authority.
Culturally, the Romans were eclectic, absorbing and adapting elements from the civilizations they encountered, particularly the Greeks. Roman art, literature, and philosophy reflected this synthesis, creating a rich cultural tapestry. Latin, the Roman language, became the lingua franca of the Western world, influencing numerous modern languages.
Roman architecture and engineering achievements were monumental. They perfected the arch, vault, and dome, constructing enduring structures like the Colosseum, Pantheon, and aqueducts. These engineering marvels not only showcased Roman ingenuity but also served practical purposes, from public entertainment to water supply.
How to Create Map Views in the Odoo 17 ERPCeline George
The map views are useful for providing a geographical representation of data. They allow users to visualize and analyze the data in a more intuitive manner.
The French Revolution, which began in 1789, was a period of radical social and political upheaval in France. It marked the decline of absolute monarchies, the rise of secular and democratic republics, and the eventual rise of Napoleon Bonaparte. This revolutionary period is crucial in understanding the transition from feudalism to modernity in Europe.
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Model Attribute Check Company Auto PropertyCeline George
In Odoo, the multi-company feature allows you to manage multiple companies within a single Odoo database instance. Each company can have its own configurations while still sharing common resources such as products, customers, and suppliers.
The Indian economy is classified into different sectors to simplify the analysis and understanding of economic activities. For Class 10, it's essential to grasp the sectors of the Indian economy, understand their characteristics, and recognize their importance. This guide will provide detailed notes on the Sectors of the Indian Economy Class 10, using specific long-tail keywords to enhance comprehension.
For more information, visit-www.vavaclasses.com
How libraries can support authors with open access requirements for UKRI fund...
20 Apr 9 Nuclear, Strong Force, Fission With Brainstorming
1. Today: More about half-life, why atoms are radioactive, fission Diagram of neutron-induced U-235 fission
2. Half-life is the average amount of time for ½ of the atoms to decay 100% remaining 50% remaining 25% remaining 12.5% remaining Time Isotope with long half-life Isotope with short half-life “ Exponential Decay”
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5. Why are some atoms radioactive? First: Some brainstorming Form small groups, with a spokesperson How many different forces in nature can you think of? Can you classify them into similar groups?
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14. Why are some atoms radioactive? The nuclear (residual strong) force presents an activation barrier Quantum mechanics allows some probability that an alpha particle can “tunnel” through the barrier Once through, electrostatic force dominates (imagine ripping apart velcro)
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17. As nuclei get larger, electrostatic force “wins” Strong force large between close protons. Strong force much lower between distal protons But electrostatic force still very high! (Nucleons on the surface feel less strong attraction.)
18. You can imagine large nuclei like large soap bubbles…very floppy Small Medium Large