This document discusses electric circuits and concepts related to current, voltage, and resistance. It contains the following key points:
1. It defines basic circuit concepts like current, charge, drift velocity, and explains how current is related to charge, time, and resistance.
2. It provides formulas for calculating current, charge, and resistance and applies them in examples. Current is calculated using charge divided by time. Resistance depends on resistivity, length, and cross-sectional area of a material.
3. It discusses series and parallel circuits, explaining how current and voltage are distributed in each type. In series circuits, current is the same but voltage adds up. In parallel, voltage is the same but current splits
The document summarizes key concepts about electricity and electrical circuits. It discusses:
1) Direct current (DC) and alternating current (AC), explaining the difference between constant and varying current over time.
2) Transformers, describing how they work by electromagnetic induction to change voltage and current levels while transmitting power.
3) Circuit parameters like voltage, current, resistance and power in AC circuits. Formulas are given relating peak, RMS and average values.
4) Waveforms of voltage, current and power over time in an AC circuit, showing their sinusoidal variation and phase relationship.
In 3 sentences or less, the document provides an overview of basic electrical concepts like different current types, transformer
1. Electric fields are produced by electric charges and can be calculated using Coulomb's law. Positive charges produce outward electric fields while negative charges produce inward electric fields.
2. The electric field strength is directly proportional to the magnitude of the charge producing the field and inversely proportional to the distance from that charge.
3. Electric potential difference is equal to the work done moving a test charge between two points in an electric field, and is calculated by multiplying the charge by the potential.
The document provides tips and information about radioactive decay and half-life calculations in 3 sections. It defines key concepts like activity, half-life, and decay equations. Examples are given for common radioisotopes like Co-60 and I-131. Steps are outlined for calculations involving initial activity, remaining activity, and decay over time. Nuclear reactions and mass-energy equivalents are also briefly discussed.
The document summarizes concepts related to forces and motion. It defines key terms like work, kinetic energy, and potential energy. It provides formulas for calculating work, kinetic energy, and gravitational potential energy. Examples are given to demonstrate applying the concepts and formulas to solve physics problems involving changes in kinetic and potential energy.
1. The document discusses the principles of refraction of light through spherical lenses and thin lenses. It defines terms such as focal length, focal point, radius of curvature, and refractive index.
2. Formulas are provided relating refractive index, angles of incidence and refraction, and focal lengths for different lens materials.
3. Worked examples apply the formulas to calculate focal lengths, refractive indices, angles of refraction and incidence, and image distances for various lens configurations and materials.
1. The document discusses simple harmonic motion (SHM) and describes the sinusoidal function y=Asin(ωt) that models SHM.
2. Various examples of SHM are shown, including spring oscillations and waves on a string. The key parameters like amplitude, angular frequency, and period are defined.
3. Standing waves on a string are analyzed, with nodes and antinodes labeled according to the quantization condition that the string length must be an integer multiple of half wavelengths. Formulas for calculating wavelength and frequency are provided.
1. The document discusses projectile motion and provides equations to calculate the time, height, horizontal displacement, and velocity of a projectile over time given the initial velocity and angle of launch.
2. Formulas are derived for calculating time, maximum height, and horizontal displacement of a projectile based on the initial velocity components along x and y axes.
3. Examples are provided to demonstrate how to apply the equations to different launch angles like 45 degrees, 60 degrees, and 30 degrees.
The document summarizes key concepts about electricity and electrical circuits. It discusses:
1) Direct current (DC) and alternating current (AC), explaining the difference between constant and varying current over time.
2) Transformers, describing how they work by electromagnetic induction to change voltage and current levels while transmitting power.
3) Circuit parameters like voltage, current, resistance and power in AC circuits. Formulas are given relating peak, RMS and average values.
4) Waveforms of voltage, current and power over time in an AC circuit, showing their sinusoidal variation and phase relationship.
In 3 sentences or less, the document provides an overview of basic electrical concepts like different current types, transformer
1. Electric fields are produced by electric charges and can be calculated using Coulomb's law. Positive charges produce outward electric fields while negative charges produce inward electric fields.
2. The electric field strength is directly proportional to the magnitude of the charge producing the field and inversely proportional to the distance from that charge.
3. Electric potential difference is equal to the work done moving a test charge between two points in an electric field, and is calculated by multiplying the charge by the potential.
The document provides tips and information about radioactive decay and half-life calculations in 3 sections. It defines key concepts like activity, half-life, and decay equations. Examples are given for common radioisotopes like Co-60 and I-131. Steps are outlined for calculations involving initial activity, remaining activity, and decay over time. Nuclear reactions and mass-energy equivalents are also briefly discussed.
The document summarizes concepts related to forces and motion. It defines key terms like work, kinetic energy, and potential energy. It provides formulas for calculating work, kinetic energy, and gravitational potential energy. Examples are given to demonstrate applying the concepts and formulas to solve physics problems involving changes in kinetic and potential energy.
1. The document discusses the principles of refraction of light through spherical lenses and thin lenses. It defines terms such as focal length, focal point, radius of curvature, and refractive index.
2. Formulas are provided relating refractive index, angles of incidence and refraction, and focal lengths for different lens materials.
3. Worked examples apply the formulas to calculate focal lengths, refractive indices, angles of refraction and incidence, and image distances for various lens configurations and materials.
1. The document discusses simple harmonic motion (SHM) and describes the sinusoidal function y=Asin(ωt) that models SHM.
2. Various examples of SHM are shown, including spring oscillations and waves on a string. The key parameters like amplitude, angular frequency, and period are defined.
3. Standing waves on a string are analyzed, with nodes and antinodes labeled according to the quantization condition that the string length must be an integer multiple of half wavelengths. Formulas for calculating wavelength and frequency are provided.
1. The document discusses projectile motion and provides equations to calculate the time, height, horizontal displacement, and velocity of a projectile over time given the initial velocity and angle of launch.
2. Formulas are derived for calculating time, maximum height, and horizontal displacement of a projectile based on the initial velocity components along x and y axes.
3. Examples are provided to demonstrate how to apply the equations to different launch angles like 45 degrees, 60 degrees, and 30 degrees.
1) The document discusses concepts related to electricity including direct current (DC), alternating current (AC), transformers, and power calculations.
2) It explains Faraday's law of induction and how changing magnetic fields can induce electromotive forces and currents.
3) Formulas are provided for calculating power in DC circuits, current and voltage ratios in transformers, and the relationships between current, voltage, and power in AC circuits.
This document provides information about electric fields and potential. Key points include:
- Electric field strength E is defined as force per unit charge, and depends on the charge Q and distance r from the charge as E=kQ/r^2
- Electric potential V at a point is defined as the work required to move a unit positive charge from infinity to that point without acceleration, and depends on charge Q and distance r as V=kQ/r
- Electric potential difference ΔV between two points is equal to the work required per unit charge to move the charge between those points.
1) The document provides various physics constants and formulas.
2) Example calculations are shown such as calculating the work done by a force and solving kinematics equations.
3) Physics concepts involving forces, kinematics, energy, and circuits are demonstrated.
1) The document provides various physics constants and formulas.
2) Example calculations are shown such as calculating the work done by a force and solving mechanics problems involving forces, displacement, velocity, and acceleration.
3) Formulas are applied to calculate values such as time, velocity, displacement, work, and more.
1. This document discusses concepts of work, energy, and power in mechanics. It provides examples of calculating work done by forces, kinetic energy, potential energy, and power for various systems.
2. Formulas and concepts are explained for work, kinetic energy, gravitational potential energy, elastic potential energy, and the work-energy theorem.
3. Several multi-part word problems are worked through step-by-step applying these formulas and concepts to calculate requested values like work, energy, acceleration, distance, and power. Diagrams accompany some examples.
1. The document defines angular displacement (θ), angular velocity (ω), and angular acceleration (α) and provides equations relating them.
2. Equations of motion are given for linear and angular variables including relationships between displacement (s), velocity (v), acceleration (a), angular displacement (θ), angular velocity (ω), and angular acceleration (α).
3. Formulas are provided for torque (τ), moment of inertia (I), and kinetic energy (Ek) in rotational motion. Sample problems are worked through applying these concepts and equations.
1. The document discusses the principles of refraction of light, including Snell's law and the relationship between the indices of refraction and angles of incidence and refraction.
2. Examples are provided to demonstrate calculating unknown values like angles and speeds given information about the indices of refraction of different media and angles of incidence or refraction.
3. The final examples show using Snell's law and relationships between trigonometric functions to calculate unknown values like the distance between two points when the refractive indices and angles are known.
1. The document discusses standing waves on a string fixed at both ends.
2. The locations of antinodes (An) and nodes (Nn) are determined by the path difference formula, where the path difference must be equal to integer or half-integer wavelengths.
3. Several examples are given of calculating the specific antinode or node locations based on given string lengths (s1 and s2) from one end.
This document discusses concepts related to forces and motion, including Newton's laws of motion. It defines key terms like force, mass, weight, friction. Examples are provided to demonstrate calculating unknown values like acceleration, force, coefficient of friction using the equations of motion. Diagrams and step-by-step working are included to illustrate problem solving. Concepts covered include calculating net force, resolving forces into components, and determining static and kinetic friction forces.
This document discusses concepts related to forces and motion, including Newton's laws of motion. It defines key terms like force, mass, weight, friction. Examples are provided to demonstrate calculating unknown values like acceleration, force, coefficient of friction using the equations of motion. Diagrams and step-by-step working are included to illustrate problem solving. Concepts covered include calculating net force, resolving forces into components, and determining static and kinetic friction forces.
1. The document discusses the physics of sound waves, including speed of sound, frequency, wavelength, and how these properties relate through equations.
2. Examples are provided to demonstrate calculating speed, frequency, and wavelength in different scenarios, as well as how observed properties change based on the motion of the source and observer.
3. Key concepts covered include the relationship between speed, frequency, and wavelength, and how the Doppler effect changes the observed frequency based on relative motion between source and observer.
1. The document provides examples of solving physics problems involving momentum and impulse using equations such as the momentum equation (∑p=∑p), the impulse-momentum theorem (Δp=FΔt), and kinematic equations.
2. Various problems are worked through step-by-step involving calculating momentum, impulse, force, velocity, and time in collisions or situations with applied forces.
3. The last examples involve solving for velocities in situations with two objects colliding or interacting, using the principle of conservation of momentum (∑p=∑p).
1. This document provides information on mechanics, including forces, moments, equilibrium conditions, stress, strain, and Young's modulus. It includes 13 examples applying these concepts to solve mechanics problems.
2. Key concepts covered include Newton's laws of motion, torque, conditions for translational and rotational equilibrium, definitions of stress and strain, and the relationship between stress, strain, and Young's modulus.
3. Formulas and step-by-step solutions are provided for problems involving forces, torques, stress, strain, and material properties.
The document discusses concepts related to kinematics including displacement (s), velocity (v), acceleration (a), and time (t). Various kinematics equations are presented and worked examples are provided to calculate values like average velocity (vav) and average acceleration (aav) given information about displacement, initial/final velocities, and time. Graphs are also used to represent relationships between variables and derive slope and equations of lines.
1. The document discusses projectile motion equations and concepts such as displacement, velocity, acceleration due to gravity, and time of flight. Equations for displacement, velocity, and time of flight are presented.
2. Examples are given of calculating time of flight, maximum displacement, velocity, and angle of projection for various projectile motion scenarios involving different initial velocities and angles.
3. Centripetal force is introduced and explained in terms of force, mass, velocity, radius, period, frequency, and angular velocity. Equations relating these quantities are provided.
This document provides information about units, prefixes, and formulas in the metric system. It includes:
1. Explanations of the seven base SI units - meter, kilogram, second, ampere, kelvin, mole, and candela.
2. Descriptions of the prefixes used to denote powers of ten when multiplying or dividing units, such as kilo (103) and milli (10-3).
3. Examples of calculations using prefixes to convert between units, like converting 4,700,000,000 meters to 4,700 kilometers.
The document also contains sections on error analysis in measurements, kinematic formulas, and dimensional analysis.
This document provides information about units, prefixes, and scientific notation used in the metric system. It defines the seven base SI units for mass, length, time, electric current, temperature, amount of substance, and luminous intensity. It also describes the prefixes that are multiplied with the base units to indicate decimal multiples and submultiples, such as kilo, mega, milli, and micro. Several examples are provided to demonstrate converting between numeric values and scientific notation with prefixes.
This document provides information about fluid statics and fluid dynamics. It defines density, calculates the density of a spherical object, and derives equations for pressure due to depth in a fluid. Examples are given for calculating pressure, force, and height in various fluid static scenarios. Fluid flow concepts such as viscosity, shear stress, and drag force are also introduced. An example problem calculates the drag force on a sphere moving through a fluid.
The document describes diffraction gratings and the diffraction of light. It contains the following key points:
1) Light passing through a diffraction grating will diffract into discrete angles based on the grating's spacing and the wavelength of light. The diffraction angles follow specific mathematical relationships.
2) Examples are provided to demonstrate calculating diffraction angles and wavelengths using these relationships for different grating spacings and wavelengths of incident light.
3) Different cases are examined for transmission and reflection gratings, and the equations for calculating diffraction angles and wavelengths are given for each case.
This document discusses concepts related to the gas laws including:
1. Definitions of key terms like pressure, volume, temperature, moles, and the gas constant R.
2. Equations relating these variables like the ideal gas law PV=nRT and how pressure, volume, and temperature are directly proportional while temperature and moles are directly proportional.
3. Explanations of how the gas laws can be used to calculate heat, work, internal energy, and other thermodynamic properties of gases.
1) The document discusses concepts related to electricity including direct current (DC), alternating current (AC), transformers, and power calculations.
2) It explains Faraday's law of induction and how changing magnetic fields can induce electromotive forces and currents.
3) Formulas are provided for calculating power in DC circuits, current and voltage ratios in transformers, and the relationships between current, voltage, and power in AC circuits.
This document provides information about electric fields and potential. Key points include:
- Electric field strength E is defined as force per unit charge, and depends on the charge Q and distance r from the charge as E=kQ/r^2
- Electric potential V at a point is defined as the work required to move a unit positive charge from infinity to that point without acceleration, and depends on charge Q and distance r as V=kQ/r
- Electric potential difference ΔV between two points is equal to the work required per unit charge to move the charge between those points.
1) The document provides various physics constants and formulas.
2) Example calculations are shown such as calculating the work done by a force and solving kinematics equations.
3) Physics concepts involving forces, kinematics, energy, and circuits are demonstrated.
1) The document provides various physics constants and formulas.
2) Example calculations are shown such as calculating the work done by a force and solving mechanics problems involving forces, displacement, velocity, and acceleration.
3) Formulas are applied to calculate values such as time, velocity, displacement, work, and more.
1. This document discusses concepts of work, energy, and power in mechanics. It provides examples of calculating work done by forces, kinetic energy, potential energy, and power for various systems.
2. Formulas and concepts are explained for work, kinetic energy, gravitational potential energy, elastic potential energy, and the work-energy theorem.
3. Several multi-part word problems are worked through step-by-step applying these formulas and concepts to calculate requested values like work, energy, acceleration, distance, and power. Diagrams accompany some examples.
1. The document defines angular displacement (θ), angular velocity (ω), and angular acceleration (α) and provides equations relating them.
2. Equations of motion are given for linear and angular variables including relationships between displacement (s), velocity (v), acceleration (a), angular displacement (θ), angular velocity (ω), and angular acceleration (α).
3. Formulas are provided for torque (τ), moment of inertia (I), and kinetic energy (Ek) in rotational motion. Sample problems are worked through applying these concepts and equations.
1. The document discusses the principles of refraction of light, including Snell's law and the relationship between the indices of refraction and angles of incidence and refraction.
2. Examples are provided to demonstrate calculating unknown values like angles and speeds given information about the indices of refraction of different media and angles of incidence or refraction.
3. The final examples show using Snell's law and relationships between trigonometric functions to calculate unknown values like the distance between two points when the refractive indices and angles are known.
1. The document discusses standing waves on a string fixed at both ends.
2. The locations of antinodes (An) and nodes (Nn) are determined by the path difference formula, where the path difference must be equal to integer or half-integer wavelengths.
3. Several examples are given of calculating the specific antinode or node locations based on given string lengths (s1 and s2) from one end.
This document discusses concepts related to forces and motion, including Newton's laws of motion. It defines key terms like force, mass, weight, friction. Examples are provided to demonstrate calculating unknown values like acceleration, force, coefficient of friction using the equations of motion. Diagrams and step-by-step working are included to illustrate problem solving. Concepts covered include calculating net force, resolving forces into components, and determining static and kinetic friction forces.
This document discusses concepts related to forces and motion, including Newton's laws of motion. It defines key terms like force, mass, weight, friction. Examples are provided to demonstrate calculating unknown values like acceleration, force, coefficient of friction using the equations of motion. Diagrams and step-by-step working are included to illustrate problem solving. Concepts covered include calculating net force, resolving forces into components, and determining static and kinetic friction forces.
1. The document discusses the physics of sound waves, including speed of sound, frequency, wavelength, and how these properties relate through equations.
2. Examples are provided to demonstrate calculating speed, frequency, and wavelength in different scenarios, as well as how observed properties change based on the motion of the source and observer.
3. Key concepts covered include the relationship between speed, frequency, and wavelength, and how the Doppler effect changes the observed frequency based on relative motion between source and observer.
1. The document provides examples of solving physics problems involving momentum and impulse using equations such as the momentum equation (∑p=∑p), the impulse-momentum theorem (Δp=FΔt), and kinematic equations.
2. Various problems are worked through step-by-step involving calculating momentum, impulse, force, velocity, and time in collisions or situations with applied forces.
3. The last examples involve solving for velocities in situations with two objects colliding or interacting, using the principle of conservation of momentum (∑p=∑p).
1. This document provides information on mechanics, including forces, moments, equilibrium conditions, stress, strain, and Young's modulus. It includes 13 examples applying these concepts to solve mechanics problems.
2. Key concepts covered include Newton's laws of motion, torque, conditions for translational and rotational equilibrium, definitions of stress and strain, and the relationship between stress, strain, and Young's modulus.
3. Formulas and step-by-step solutions are provided for problems involving forces, torques, stress, strain, and material properties.
The document discusses concepts related to kinematics including displacement (s), velocity (v), acceleration (a), and time (t). Various kinematics equations are presented and worked examples are provided to calculate values like average velocity (vav) and average acceleration (aav) given information about displacement, initial/final velocities, and time. Graphs are also used to represent relationships between variables and derive slope and equations of lines.
1. The document discusses projectile motion equations and concepts such as displacement, velocity, acceleration due to gravity, and time of flight. Equations for displacement, velocity, and time of flight are presented.
2. Examples are given of calculating time of flight, maximum displacement, velocity, and angle of projection for various projectile motion scenarios involving different initial velocities and angles.
3. Centripetal force is introduced and explained in terms of force, mass, velocity, radius, period, frequency, and angular velocity. Equations relating these quantities are provided.
This document provides information about units, prefixes, and formulas in the metric system. It includes:
1. Explanations of the seven base SI units - meter, kilogram, second, ampere, kelvin, mole, and candela.
2. Descriptions of the prefixes used to denote powers of ten when multiplying or dividing units, such as kilo (103) and milli (10-3).
3. Examples of calculations using prefixes to convert between units, like converting 4,700,000,000 meters to 4,700 kilometers.
The document also contains sections on error analysis in measurements, kinematic formulas, and dimensional analysis.
This document provides information about units, prefixes, and scientific notation used in the metric system. It defines the seven base SI units for mass, length, time, electric current, temperature, amount of substance, and luminous intensity. It also describes the prefixes that are multiplied with the base units to indicate decimal multiples and submultiples, such as kilo, mega, milli, and micro. Several examples are provided to demonstrate converting between numeric values and scientific notation with prefixes.
This document provides information about fluid statics and fluid dynamics. It defines density, calculates the density of a spherical object, and derives equations for pressure due to depth in a fluid. Examples are given for calculating pressure, force, and height in various fluid static scenarios. Fluid flow concepts such as viscosity, shear stress, and drag force are also introduced. An example problem calculates the drag force on a sphere moving through a fluid.
The document describes diffraction gratings and the diffraction of light. It contains the following key points:
1) Light passing through a diffraction grating will diffract into discrete angles based on the grating's spacing and the wavelength of light. The diffraction angles follow specific mathematical relationships.
2) Examples are provided to demonstrate calculating diffraction angles and wavelengths using these relationships for different grating spacings and wavelengths of incident light.
3) Different cases are examined for transmission and reflection gratings, and the equations for calculating diffraction angles and wavelengths are given for each case.
This document discusses concepts related to the gas laws including:
1. Definitions of key terms like pressure, volume, temperature, moles, and the gas constant R.
2. Equations relating these variables like the ideal gas law PV=nRT and how pressure, volume, and temperature are directly proportional while temperature and moles are directly proportional.
3. Explanations of how the gas laws can be used to calculate heat, work, internal energy, and other thermodynamic properties of gases.
(June 12, 2024) Webinar: Development of PET theranostics targeting the molecu...Scintica Instrumentation
Targeting Hsp90 and its pathogen Orthologs with Tethered Inhibitors as a Diagnostic and Therapeutic Strategy for cancer and infectious diseases with Dr. Timothy Haystead.
PPT on Direct Seeded Rice presented at the three-day 'Training and Validation Workshop on Modules of Climate Smart Agriculture (CSA) Technologies in South Asia' workshop on April 22, 2024.
Authoring a personal GPT for your research and practice: How we created the Q...Leonel Morgado
Thematic analysis in qualitative research is a time-consuming and systematic task, typically done using teams. Team members must ground their activities on common understandings of the major concepts underlying the thematic analysis, and define criteria for its development. However, conceptual misunderstandings, equivocations, and lack of adherence to criteria are challenges to the quality and speed of this process. Given the distributed and uncertain nature of this process, we wondered if the tasks in thematic analysis could be supported by readily available artificial intelligence chatbots. Our early efforts point to potential benefits: not just saving time in the coding process but better adherence to criteria and grounding, by increasing triangulation between humans and artificial intelligence. This tutorial will provide a description and demonstration of the process we followed, as two academic researchers, to develop a custom ChatGPT to assist with qualitative coding in the thematic data analysis process of immersive learning accounts in a survey of the academic literature: QUAL-E Immersive Learning Thematic Analysis Helper. In the hands-on time, participants will try out QUAL-E and develop their ideas for their own qualitative coding ChatGPT. Participants that have the paid ChatGPT Plus subscription can create a draft of their assistants. The organizers will provide course materials and slide deck that participants will be able to utilize to continue development of their custom GPT. The paid subscription to ChatGPT Plus is not required to participate in this workshop, just for trying out personal GPTs during it.
PPT on Alternate Wetting and Drying presented at the three-day 'Training and Validation Workshop on Modules of Climate Smart Agriculture (CSA) Technologies in South Asia' workshop on April 22, 2024.
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
ESA/ACT Science Coffee: Diego Blas - Gravitational wave detection with orbita...Advanced-Concepts-Team
Presentation in the Science Coffee of the Advanced Concepts Team of the European Space Agency on the 07.06.2024.
Speaker: Diego Blas (IFAE/ICREA)
Title: Gravitational wave detection with orbital motion of Moon and artificial
Abstract:
In this talk I will describe some recent ideas to find gravitational waves from supermassive black holes or of primordial origin by studying their secular effect on the orbital motion of the Moon or satellites that are laser ranged.
Anti-Universe And Emergent Gravity and the Dark UniverseSérgio Sacani
Recent theoretical progress indicates that spacetime and gravity emerge together from the entanglement structure of an underlying microscopic theory. These ideas are best understood in Anti-de Sitter space, where they rely on the area law for entanglement entropy. The extension to de Sitter space requires taking into account the entropy and temperature associated with the cosmological horizon. Using insights from string theory, black hole physics and quantum information theory we argue that the positive dark energy leads to a thermal volume law contribution to the entropy that overtakes the area law precisely at the cosmological horizon. Due to the competition between area and volume law entanglement the microscopic de Sitter states do not thermalise at sub-Hubble scales: they exhibit memory effects in the form of an entropy displacement caused by matter. The emergent laws of gravity contain an additional ‘dark’ gravitational force describing the ‘elastic’ response due to the entropy displacement. We derive an estimate of the strength of this extra force in terms of the baryonic mass, Newton’s constant and the Hubble acceleration scale a0 = cH0, and provide evidence for the fact that this additional ‘dark gravity force’ explains the observed phenomena in galaxies and clusters currently attributed to dark matter.
When I was asked to give a companion lecture in support of ‘The Philosophy of Science’ (https://shorturl.at/4pUXz) I decided not to walk through the detail of the many methodologies in order of use. Instead, I chose to employ a long standing, and ongoing, scientific development as an exemplar. And so, I chose the ever evolving story of Thermodynamics as a scientific investigation at its best.
Conducted over a period of >200 years, Thermodynamics R&D, and application, benefitted from the highest levels of professionalism, collaboration, and technical thoroughness. New layers of application, methodology, and practice were made possible by the progressive advance of technology. In turn, this has seen measurement and modelling accuracy continually improved at a micro and macro level.
Perhaps most importantly, Thermodynamics rapidly became a primary tool in the advance of applied science/engineering/technology, spanning micro-tech, to aerospace and cosmology. I can think of no better a story to illustrate the breadth of scientific methodologies and applications at their best.
The cost of acquiring information by natural selectionCarl Bergstrom
This is a short talk that I gave at the Banff International Research Station workshop on Modeling and Theory in Population Biology. The idea is to try to understand how the burden of natural selection relates to the amount of information that selection puts into the genome.
It's based on the first part of this research paper:
The cost of information acquisition by natural selection
Ryan Seamus McGee, Olivia Kosterlitz, Artem Kaznatcheev, Benjamin Kerr, Carl T. Bergstrom
bioRxiv 2022.07.02.498577; doi: https://doi.org/10.1101/2022.07.02.498577
CLASS 12th CHEMISTRY SOLID STATE ppt (Animated)eitps1506
Description:
Dive into the fascinating realm of solid-state physics with our meticulously crafted online PowerPoint presentation. This immersive educational resource offers a comprehensive exploration of the fundamental concepts, theories, and applications within the realm of solid-state physics.
From crystalline structures to semiconductor devices, this presentation delves into the intricate principles governing the behavior of solids, providing clear explanations and illustrative examples to enhance understanding. Whether you're a student delving into the subject for the first time or a seasoned researcher seeking to deepen your knowledge, our presentation offers valuable insights and in-depth analyses to cater to various levels of expertise.
Key topics covered include:
Crystal Structures: Unravel the mysteries of crystalline arrangements and their significance in determining material properties.
Band Theory: Explore the electronic band structure of solids and understand how it influences their conductive properties.
Semiconductor Physics: Delve into the behavior of semiconductors, including doping, carrier transport, and device applications.
Magnetic Properties: Investigate the magnetic behavior of solids, including ferromagnetism, antiferromagnetism, and ferrimagnetism.
Optical Properties: Examine the interaction of light with solids, including absorption, reflection, and transmission phenomena.
With visually engaging slides, informative content, and interactive elements, our online PowerPoint presentation serves as a valuable resource for students, educators, and enthusiasts alike, facilitating a deeper understanding of the captivating world of solid-state physics. Explore the intricacies of solid-state materials and unlock the secrets behind their remarkable properties with our comprehensive presentation.
The debris of the ‘last major merger’ is dynamically youngSérgio Sacani
The Milky Way’s (MW) inner stellar halo contains an [Fe/H]-rich component with highly eccentric orbits, often referred to as the
‘last major merger.’ Hypotheses for the origin of this component include Gaia-Sausage/Enceladus (GSE), where the progenitor
collided with the MW proto-disc 8–11 Gyr ago, and the Virgo Radial Merger (VRM), where the progenitor collided with the
MW disc within the last 3 Gyr. These two scenarios make different predictions about observable structure in local phase space,
because the morphology of debris depends on how long it has had to phase mix. The recently identified phase-space folds in Gaia
DR3 have positive caustic velocities, making them fundamentally different than the phase-mixed chevrons found in simulations
at late times. Roughly 20 per cent of the stars in the prograde local stellar halo are associated with the observed caustics. Based
on a simple phase-mixing model, the observed number of caustics are consistent with a merger that occurred 1–2 Gyr ago.
We also compare the observed phase-space distribution to FIRE-2 Latte simulations of GSE-like mergers, using a quantitative
measurement of phase mixing (2D causticality). The observed local phase-space distribution best matches the simulated data
1–2 Gyr after collision, and certainly not later than 3 Gyr. This is further evidence that the progenitor of the ‘last major merger’
did not collide with the MW proto-disc at early times, as is thought for the GSE, but instead collided with the MW disc within
the last few Gyr, consistent with the body of work surrounding the VRM.
2. F ˆ F www.schoolDD.com 1
16
16.1 ˂
˂ (electric current) ˂
F ˂
ˈ ˂ . F F
ˈ F F F F
F F F F
ˈ . ˂
˂ F F F
F F ˂ F F F ˂
F F F ˂ F F F F F ˂ F F F
F ˂ F F F F ˂ F F
F ˂ F F F F F ˂ ˈ F
16.1.1 ˂
˂ ˂ F ˂
˂
ˈ ˂ (free electron) F F
F F F F F F (Brownian motion)
F ˈ F
ˈ
..
3. F ˆ F www.schoolDD.com 2
F F F F ˂ F
˂ F F ˈ F
(drift velocity) F ˂ F ˂
16.1.2 ˂ ˂
˂ ˂ F F
˂
˂ F F ˂ F
F ˈ F F ˈ F F F (A)
I = ˂ (A)
Q = ( ) F (C)
t = F (s)
˂ I ˂ E
F 1
F ˂ 1.25 F F F F F F
F 5 F F
I =
ۿ
ܜ
F
F F
F F F ˂ (VA = VB)
F
F F F F ˂
(VB > VA) ˂ F
˂
VA = VB
VA VB
VB > VA
VA VB
4. F ˆ F www.schoolDD.com 3
F 2
F F F F ˂ F F 3.2 F
F F 5.0 ( ˂ 1.6 X10-19
F)
˂
F F ˂
s = vt
I = 1.25 A
II
I = 3.2 A
t = 5 , Q = ?
˂ I =
୕
୲
Q = It
= 1.25x5.0
Q = 6.25 C Ans
˂ I =
୕
୲
Q = It
Q = 3.2x5.0 C
F 1 1.6 X10-19
C
= ଷ.ଶ୶ହ.
ଵ.௫ଵషభవ
= 1x1020
Ans
I
E
˂ , F E
˂ (I)
F
5. F ˆ F www.schoolDD.com 4
˂ I =
୕
୲
˂ Q = Ne = (nAs)e = (nAvt)e = nevtA
I =
୬ୣ୴୲
୲
I = nevA
n = F ( / m3
)
e = (1.6 x 10- 19
C)
v = (m/s)
A = (m2
)
F 3
F 5.0 x 1028
F F F 2.5 F
F F 0.30 F ˂ F
F
16.2 F F ˂ (I) F F (V)
16.2.1 F F
˂ F F F F ˂ F
I ן V
I = KV ( K = F )
୍
=
ଵ
୍
= R (
ଵ
= R)
R = F F ˈ F F F F ( Ω )
V = I R F
A = 2.5x10-6
m2
n = 5x1028
v = 0.3x10-3
m/s
I = ? I = nevA
= 5x1028
x1.6x10-19
x0.3x10-3
x2.5x10-6
I = 6.0 A Ans
.
6. F ˆ F www.schoolDD.com 5
- F F F ˈ F
F 4
F F F F ˂ ˈ F F
F 5
F F F 1.0 F F F F ˂ 1.0 F F
F F
F (Resistor)
F ˈ F F F F ˂ F F ˂ F
F 2
1. F (Fixed resistor) F F ˈ F
F F F ˂ F F F
V
I
V
I
F
V
I
V
I
3
2
1
0 0.2 0.4 0.6
I (A)
V (V)
F V = IR
= 1x10-3
x1x106
V = 1x103
V Ans
V = ?
I
R = 1x106
Ω
I = 1x10-3
A
7. F ˆ F www.schoolDD.com 6
1 2 3 4
F
0 0 1 -
1 1 101
േ 1 %
2 2 102
േ 2 %
F 3 3 103
-
4 4 104
-
5 5 105
-
6 6 106
-
F 7 7 - -
8 8 - -
9 9 - -
- - 10-1
േ 5 %
- - 10-2
േ 10 %
2. F F (Variable resistor) ˈ F F F F F
˂ F F F F F
F F 1 3 F F 2 F F ˂
(Diode)
ˈ F F F F F
˂ ˂ ˂
F ˂ 2
F
2
F F
31
A
FI A FF A
F F 2
F 1 F 3 F
F F
F ˂ F F ˂
4 F
1
2
3
4 ˈ F
F F
F 15x103
F
േ2 % F 15,000 F േ
300 F F F 14,700 F
15,300 F
8. F ˆ F www.schoolDD.com 7
- F ˂ F F F ˂ ˈ ˂
F 6
F a F F b F F C
F F F F
F a F = 30x102
Ω േ 150 Ω
F b F = 18x103
Ω േ 1800 Ω
F c F =
16.2.2 F ˂
F ˂ ߩ ˈ F F
˂ F F F F F F ˂
F ˈ F
F F F F ˂ (V) ˂ (I) F
(R) F F
୍
ן
ℓ
R ן
ℓ
F F ߩ = 1.6x10-8
Ω m , ߩ = 1.7x10-8
Ω m
ߩ F = 1010
- 1014
Ω m , ߩ = 1014
- 1018
Ω m
F 7
F 10 F F F F 1 F
F F F 2 F F F ˈ F F
F ( ߩ = 1.7x10-8
Ω m)
1 8 103
േ 10%
3 0 102
േ 5%
R =
࣋र
ۯ
F
F
. F
ߩ F F ˂
9. F ˆ F www.schoolDD.com 8
F
F
R =
ఘℓ
R1 =
ଵ.୶ଵషఴ୶ଵ
.଼ହ୶ଵషళ
R1 = 0.216 Ω Ans
F
F
R =
ఘℓ
R2 =
ଵ.୶ଵషఴ୶ଵ
ଷ.ଵସ୶ଵషల
R2 = 0.054 Ω Ans
ୖభ
ୖమ
=
.ଶଵ
.ହସ
= 4
1 F F 2 F 4 F Ans
˂ G ˈ F F ˂ F ˈ ( F )-1
F (S)
G =
ଵ
ୖ
˂ ߪ ˈ ˈ F F ˂ F ˈ
( F )-1
F F (S/m)
ߪ =
ଵ
ఘ
16.2.3 F F
ˈ F F F
T ---> R
F F F F F
T ---> R
ˈ F F
T ---> R
A =
గௗమ
ସ
=
ଷ.ଵସ୶ሺଵ୶ଵషయሻమ
ସ
= 7.85x10-7
m2
d = 1x10-3
m
ℓ = 10 m
A =
గௗమ
ସ
=
ଷ.ଵସ୶ሺଶ୶ଵషయሻమ
ସ
= 3.14x10-6
m2
d = 2x10-3
m
ℓ = 10 m
10. F ˆ F www.schoolDD.com 9
(Superconductivity) F ˂ ˈ F (ߩ = 0) F
F (critical temperature) F (Supper
conductor)
16.3 ˂
16.3.1 ˂ ( E) F F (V)
F F ˂ ( F F ) F F F F
˂ F F F ˂ ˂
F F ˂
F F F R F ˂
E F r F F ˂ I F F
˂ F ˂ ( ) F F F ˂ Q
˂ E F F F r R F F ˂ Q F F
F F
F WE = ˂ F
WR = ˂ F F R
Wr = ˂ F F r
F F F WE = WR + Wr
QE = QVR + QVr
F
I
F ˂
E I
F R
I
VR
r E
V
Vr
R
I
E = VR + Vr
I
11. F ˆ F www.schoolDD.com 10
E = IR + Ir
F I =
ሺୖା୰ሻ
F V F F F F V = VR
F V F F R F F F V ؆ E F F V = E
F 8
F ˂ 12.0 F F 2.0 F F F 7.0
F F F F F F F F F F F
F F F F F F
I E = VR + Vr
E = IR + Ir
I =
ሺୖା୰ሻ
=
ଵଶ
ሺାଶሻ
=
ଵ
A
V = VR = IR
=
ଵ
x70
V = 11.67 V Ans
F F F F
F V ؆ E = 12 V Ans
VR
r = 2 E = 12 V
V= ?
Vr
R = 20 Ω
I
r = 2 E = 12 V
V= ?
12. F ˆ F www.schoolDD.com 11
16.3.2 ˂
˂
F Q = ˂ F F t (C)
I = ˂ F F (A)
V = F F F (V)
W = ˂ F F ( J)
I =
୕
୲
Q = It V = IR
W = ItV = I2
Rt =
మ୲
ୖ
˂ P ˂ F F F ˈ F F (W)
F 9
F 1.5 F 2 F F F ˂ 20 F
F 20 F F 15 F ˂ F ˂ 1 F
˂ F W = QV
= ItV
E
I
R
I V
W = QV
P =
܅
ܜ
P =
୲
=
ItV
୲
= IV
E = 1.5x2 = 3 V
t = 20 hr
I=20 mA
13. F ˆ F www.schoolDD.com 12
= 20x10-3
x(20x60x60)x3
W = 4320 J
F ˂ F ˂ 1 F =
ଵହ୶ଶ
ସଷଶ
= 0.007 / Ans
16.4 F F
16.4.1 F F
1. F
ˈ F F F F F
F F F
- ˂ F F F
I = I1 = I2 = I3
- F F ˂ = F F ˂ F
V = V1 + V2 + V3
V = V1 + V2 + V3
V = IR ( F )
IR = I1 R1 + I2 R2 + I3R3
R = F R 1 , R 2 R 3
2. F
ˈ F F F ˈ F
R3R1 R2
I1
E
I
V
V1
I2 I3
V2 V3
R = R1 + R2 + R3
(I = I1 = I2 = I3)
14. F ˆ F www.schoolDD.com 13
F F F
- F F F F F = F F ˂
V = V1 = V2 = V3
- ˂ F = ˂ F F F
I = I1 + I2 + I3
I = I1 + I2 + I3
V = IR I =
ୖ
ୖ
=
భ
ୖభ
+
మ
ୖమ
+
య
ୖయ
R = F R1 , R2 R3
- F F F F F F F
˂ F F F F F ˂ F F
- F F ˈ F F F
F 10
F F F
. F S ʽ . F S ʽ
E
V1 = V2 = V3
R3
I I
I1
V
I3
R2
I2
R1
܀
=
܀
+
܀
+
܀
(V = V1 = V2 = V3)
15. F ˆ F www.schoolDD.com 14
. F S ʽ
F F
F R 1 R 2 F
F F R 12 = R 1 + R 2 = 1 +2 = 3 Ω
F R 3 R 4 F
F F R 34 = R 3 + R 4 = 3 +4 = 7 Ω
F F
F R 12 R 34 F
F F
ଵ
ୖ
=
ଵ
ୖభమ
+
ଵ
ୖయర
=
ଵ
ଷ
+
ଵ
=
ାଷ
ଶଵ
ଵ
ୖ
=
ଵ
ଶଵ
R = 2.1 Ω Ans
. F S ʽ
F F
F R 1 R 3 F
4 Ω3 Ω
2 Ω
B
S
1 Ω
I
A
R4R3
R2R1
4 Ω3 Ω
2 Ω
B
1 Ω
I
A
R34
R12
7 Ω
B
3 Ω
I
A
R4R3
R2R1
4 Ω3 Ω
2 Ω
B
1 Ω
I
A
16. F ˆ F www.schoolDD.com 15
F F
ଵ
ୖభయ
=
ଵ
ୖభ
+
ଵ
ୖయ
=
ଵ
ଵ
+
ଵ
ଷ
=
ଷାଵ
ଷ
ଵ
ୖభయ
=
ସ
ଷ
R13 =
ଷ
ସ
Ω
F R 2 R 4 F
F F
ଵ
ୖమర
=
ଵ
ୖమ
+
ଵ
ୖర
=
ଵ
ଶ
+
ଵ
ସ
=
ଶାଵ
ସ
ଵ
ୖమర
=
ଷ
ସ
R24 =
ସ
ଷ
Ω
F F
F R 13 R24 F
F F R = R13 + R24
=
ଷ
ସ
+
ସ
ଷ
=
ଽ ାଵ
ଵଶ
=
ଶହ
ଵଶ
R = 2.08 Ω Ans
16.4.2 F
1. F
ˈ F F F F F
F F F
- ˂ = ˂ F
F F F F
R24R13
4/3 Ω B3/4 Ω
I
A
E3r1 E1
R
I
r2 E2
r3
E = E1 + E2 + E3
17. F ˆ F www.schoolDD.com 16
2. F
ˈ F F F F
F ˂ F F F E1 = E2 = E3
F F F
- ˂ = ˂ F F F
- F F F F
- F F ˂ F F ˂
F
F 11
F F ˂ 0.25 F F F 8 F
F F ˂ 0.16 F ˂ F
F ˂ F F F F E r
r = r1 + r2 + r3
E = E1 = E2 = E3
ܚ
=
ܚ
+
ܚ
+
ܚ
E3
r2 E2
R
I r1 E1
r3
18. F ˆ F www.schoolDD.com 17
F
˂ E = E1 + E2 = E + E = 2E
F r = r1 + r2 = r + r = 2r
F F
V = E I r
V = IR
F IR = 2E I(2r)
0.25x8 = 2E 0.25(2r)
E 0.25r = 1 ---1
F
˂ E = E1 = E2 = E
F
ଵ
୰
=
ଵ
୰భ
+
ଵ
୰మ
=
ଵ
୰
+
ଵ
୰
=
ଶ
୰
r =
୰
ଶ
F F
r1 E1
R = 8 Ω
I = 0.25 A
r2 E2
V
V
r E
R = 8 Ω
I = 0.25 A
r1 E1
R = 8 Ω
I = 0.16 A
r2 E2
V
V
r E
R = 8 Ω
I = 0.16 A
19. F ˆ F www.schoolDD.com 18
V = E I r
V = IR
F IR = E I(
୰
ଶ
)
0.16x8 = E 0.16(
୰
ଶ
)
E 0.08r = 1.28 ---2
2-1, -0.08r + 0.25r = 0.28
0.17r = 0.28
r = 1.7 Ω Ans
F r 2 F E 0.08(1.7) = 1.28
E = 1.41 V Ans
16.5 F ˂ F
˂ F F ˂ F F F
F F ˂
F 12
˂ F F a , b c ˂
F E1 = 6 V , E2 = 6 V , r1 = 1 Ω , r2 = 1 Ω , Ra = 7 Ω , Rb = 4 Ω , Rc = 12 Ω
F
F b c F F F F a
F b c
ଵ
ୖౘౙ
=
ଵ
ୖౘ
+
ଵ
ୖౙ
=
ଵ
ସ
+
ଵ
ଵଶ
=
ଷାଵ
ଵଶ
=
ସ
ଵଶ
=
ଵ
ଷ
Rbc = 3 Ω
F a bc R = Ra + Rbc
= 7 + 3
R = 10 Ω
E1 E2 F
˂ E = E1 + E2 = 6 + 6 = 12 V
c
r1 E1
a
I
r2 E2
b
20. F ˆ F www.schoolDD.com 19
F r = r1 + r2 = 1 + 1 = 2 Ω
F F
V = E I r
V = IR
F IR = E I r
Ix10 = 12 Ix2
I = 1.0 A
˂ F F a , Ia = I = 1.0 A Ans
F Ia = Ib + Ic
1.0 = Ib + Ic
Ic = 1.0 - Ib
Vb = Vc
IbRb = IcRc
IbRb = (1.0 - Ib)Rc
Ibx4 = (1.0 - Ib)x12
Ib =
ଵଶ
ଵ
=
ଷ
ସ
= 0.75 A Ans
Ic = 1.0 - Ib = 1.0 - 0.75 = 0.25 A Ans
F 13
F F ˂ 10 F F F F
F F 1.2 F F F 6 F F F F
F F F F F F F
F F F ˂ 6 V.
F F F F F 1.2 V. ˂ F F 10
mA.
V
r E
R
I
21. F ˆ F www.schoolDD.com 20
0
F F F F F F F F F
F R F
V = VR + VD
V = E I r = E
F E = VR + VD
VR = E VD = 6 1.2
VR = 4.8 V
F
VR = I R
R =
୍
=
ସ.଼
ଵ௫ଵషయ
R = 480 Ω Ans
F 14
˂ ˂ 2 F F F F F F
. ˂ F
. F F F F
. F
. ˂ F 10
. ˂ F
.
˂ F F ˂ F F F
I = I = 2 A Ans
VDVR
F
V
E , r = 0
R
I
r = 0
E = 6 V
R = 0.5 Ω
R1
I = 2 A
22. F ˆ F www.schoolDD.com 21
. VR = ?
F V = I R
VR = 2x0.5
VR = 1.0 V Ans
. R1 = ?
E = I r + I R + I R1
6 = 2x0 + 2x0.5 + 2xR1
R1 =
ିଵ
ଶ
R1 = 2.5 Ω Ans
. W = ? t = 10 s
W = QV
= QE
= ItE (I =
୕
୲
)
= 2x10x6
W = 120 J Ans
. PR = ?
W = QV
P =
୲
P =
QV
୲
PR =
QVR
୲
=
ItሺIRሻ
୲
= I2
R = 22
x0.5
PR = 2 W Ans
F 15
F F F a b
R3 = 2 ΩR2 = 2 Ω
b
.
E = 9 V
R1 = 1 Ω
a
I
R2 = 2 Ω
b
.
E = 9 V
R1 = 1 Ω
a
I
23. F ˆ F www.schoolDD.com 22
0
0
. V2 = ?
V2 V2 = I R2
F R2 I
R1 R2 F
R = R1 + R2 = 1 + 2 = 3 Ω
V = I R
V = E I r
F E = I R
9 = Ix3
I = 3 A
V2 = I R2 = 3x2
V2 = 6 V Ans
. V2 = ?
R2 R3 F
F
ଵ
ୖౘ
=
ଵ
ୖమ
+
ଵ
ୖయ
=
ଵ
ଶ
+
ଵ
ଶ
Rab = 1 Ω
R1 Rab F
F R = R1 + Rab = 1 + 1 = 2 Ω
V = I R
V = E I r
F E = I R
9 = Ix2
I = 4.5 A
Vab = I Rab = 4.5x1
Vab = 4.5 V Ans
16.6 ˂
˂ F F F F F F F F
F (galvanometer) F F F
F
RE
r = 0
I
V
24. F ˆ F www.schoolDD.com 23
16.6.1 F
ˈ ˂ F F F ˂
F ˈ F F F F F (shunt) F
Rs F F F F I ˈ F F F
F F IG F F F F IS
F F F F F F F F F
F F F
VS = VG
ISRS = IGRG
F RS =
୍ృୖృ
୍
I = IG + IS
F 16
F F F F 1000 F ˂ 50 F
F ˈ F ˂ F 100 F
. F F F F
. F F ˈ F
˂ F
E , r
R
I
F
E , r
R
I
A
IG = 50ߤA RG = 1000 Ω
RS = ?
I = 100 mA
G
IS
F F F
˂ F I
F
RGIG
RS
I
G
F A
IS
G
25. F ˆ F www.schoolDD.com 24
. RS = ?
I = IG + IS
IS = I - IG
IS = 100x10-3
50x10-6
A
VS = VG ( F )
ISRS = IGRG
RS =
୍ృୖృ
୍
=
ହ୶ଵషల୶ଵ
ଵ୶ଵషయିହ୶ଵషల
=
ଵ
ଶ୶ଵయିଵ
RS = 0.5 Ω Ans
. RA = ?
ଵ
ୖఽ
=
ଵ
ୖృ
+
ଵ
ୖ
( F )
ଵ
ୖఽ
=
ଵ
ଵ
+
ଵ
.ହ
=
ଵାଶ
ଵ
=
ଵ
.ହ
RA = 0.5 Ω Ans
- F F F F F F ˂
F
16.6.2 F F
ˈ F F ˂ ˂ F F F F ˂
F ˈ F F F F F F
(multiplier) F Rm F F F F F F
F Vm F ˈ F F F F VG
F F F F R
F F ˂ F
˂ F
ba
E , r
R
I
ba
F F
E , r
R
I
V
V
G
26. F ˆ F www.schoolDD.com 25
V = Vm + VG
V = IGRm + IGRG
V = IG(Rm + RG)
Rm =
୍ృ
- RG
F F F F F F F F
F F F F F F F
F 17
F F F 16 F ˈ F F F F F 10 F
. F F F F F
. F F F F F F F F
. F F F F F
. Rm = ?
V = Vm + VG
V = IGRm + IGRG
10 = 50x10-6
xRm + 50x10-6
x1000
Rm =
ଵି.ହ
ହ୶ଵషల
Rm = 200,000 Ω Ans
F
RGIG
Rm
VG
G
Vm
F F V
RG = 1000 Ω
IG = 50 ߤA Rm = ?
VG
G
Vm
V
27. F ˆ F www.schoolDD.com 26
. F Rm = 0 , VG = ?
VG = IGRG
= 50x10-6
x1000
VG = 50x10-3
V Ans
. RV = ?
RV = Rm + RG ( F )
= 200.000 + 1000
RV = 201,000 Ω Ans
- F F F F F F ˂
F
16.6.3 F F
ˈ F F
F F F F F F F R0 E
F F Rx F x y F F
˂ F F F F F F F F ˈ F F
ˈ ˂ F F
E = Vr + VRX + VRG + VR0
E = I r + I RX + I RG + I R0
yx
F F
R
OR
F
yx
R0
RX
RG
E , r
I
G
F F O
x y
F F F
G
28. F ˆ F www.schoolDD.com 27
N
S
E = I (r + RX + RG + R0)
I =
ሺ୰ା ୖା ୖృା ୖబሻ
- x y F Rx = 0 ˂ F
( ) 0 F F F F F F x y
F 0 F F F F 0 F F F R0
0 F F F
16.7 F F ˂ F
16.7.1 F F
F (Magnet) F F F F
F F F F F
F F
1. F (magnetic pole)
F F F F F
F F
2. F
F 2 (north pole) F (south pole) F F
F F F
3. F F 2
- F F F
- F F
F
S N N S
N S S N
S N S N
F
29. F ˆ F www.schoolDD.com 28
F (magnetic field)
F F F F
F F F F
- F F F F F
- F F F F F
F
ˈ F F F F F F
ˈ F F F F F F F F F
F F F F F F F F F F F
F
N N
S
N
F
S
N
F F
x F F F F
ˈ F F ˈ F
F F
30. F ˆ F www.schoolDD.com 29
F F
F F ߔ F F F
F ˈ F (Wb)
F F F F B F F F F
F ˈ F F (T)
F 18
F F 5 x 10- 4
F F F 10 F F
F F F
F ˂ F
˂ F F F
F F F F
B =
ࢶ
ۯ
Φ = 5x10-4
Wb
A = 10x10-4
m2
A (m2
)
S N
F F ߔ (Wb)
B =
ః
=
ହ୶ଵషర
ଵ୶ଵషర
B = 0.5 T Ans
Fv+q
F F
F
v
+q
F
31. F ˆ F www.schoolDD.com 30
F F F
F = F F q (N)
q = ˂ F F (C)
V = (m/s)
B = F (T)
F (F) F F F (v)
F (B) F (F) F (+q)
(-q) F (F) F F
F 19
-1.6x 10-19
F F 1.0x 107
F F
F F 5.0 x10 -3
F
F F
F = qvB
F
B
v
+q
90°
F
B
v
-q
90°
F
Bv
v-q
˂ ˂
F = qvB
=
F = Ans
32. F ˆ F www.schoolDD.com 31
F ˂ F F F
˂ F F F F F
˂ F
F F F F =
qvB F F
F F F
F = qvB ---1
˂ I =
୯
୲
q = It
v =
ୱ
୲
=
ℓ
୲
F q v 1
F F = It(
ℓ
୲
) B
F = F (N)
I = ˂ F (A)
ℓ = (m)
B = F (T)
(F) F F F F
F ˂ F
F ˂ ( +) F
B
IN
S
ℓ
F
BI
N
S
F ˂ F F F
F = IरB
33. F ˆ F www.schoolDD.com 32
F 20
20 50 F 2 F ˂ 10
F F F F F ( F F F
)
16.7.2 ˂ F F
. F
F ˂ F F F F
F F ˂
F
I
B
I
B
F
BI
90°
F
B
I
ℓ = 0.2
F
B = 2 T
I = 10 A
N
S
F = IℓB
= 10x0.2x2
F = 4 N
F F 2
∑ F = ma
4 = 50x10-3
xa
a =
ସ
.ହ
a = 80 m/s2
Ans
F F
34. F ˆ F www.schoolDD.com 33
. F F
F ˈ ˈ F F F ˂ F F
F F F F F F F F
˂ F F F F ˈ F ˂ F F ˂ F F
F
I
B
I
I
B
I
F F F
F F
I
B
B
N S
I
35. F ˆ F www.schoolDD.com 34
16.7.3 F F ˂ F
F 2 F F F ˂ F
F F F ˂ F F F
F ˂ F F F 1 F B1
F 2 F F B1 F12 F F 2
2 F B2 F 1 F
F B2 F21 F F 1
F F F ˂ F F ˈ
F ˂ ˈ
16.7.4 F ˂ F F F
F F F ˂ F
I1
B2
F
F21 F12
B1
I2
I1
B2
F
B1
I2 I1
B2
F
B1
I2
I1
B2
F
F21
B1
I2
F12
. I . I
36. F ˆ F www.schoolDD.com 35
F F F = IℓB = IbB F F
F ˈ F F F F F
F F PS QR = a
F PQ SR = b
F F F
F F = x F
M = F (a cosθ) = IbB (a cosθ)
M = IAB cosθ ( A = axb = )
F N F
M = NIAB cosθ
F Mmax cosθ = 1 θ = 0°
Mmin cosθ = 0 θ = 90°
F 21
F 1000 F 5 8 F
F 1 F ˂ 2 F F F F
60 F
b
a
S
RQ
P
I
I
I
BB
F
F
a cosθ
F
F
a
S
θP
B
37. F ˆ F www.schoolDD.com 36
16.8 F ˂
F ˂ ˈ F ˂ ˈ
F F F ˂ F F F
F ˂
. ˂ F PQRS F F F
F F
F F F a b F x y F y
x F ˂ SRQP F F
F F .
- F F F F F F
(M=0) F ( M = F (a cosθ))
a cos60
F
F
a = 0.05
60°
B = 1 T
y x
ba
P
QR
S
I
I
I BB
F
F
N S
F F M = F (a cos60)
= IℓB (a cos60)
= 2x0.08x1.0x (0.05x0.5)
= 4x10-3
N
N = 1000
M = NM = 1000x4x10-3
M = 4.0 N-m Ans
F F ˂
yx
ba
F
S
RQ
P
I
I
I BB
F
F
N S
. .