1) The document contains solutions to physics problems involving kinetics energy (T), work (W), velocity (v), mass (m), distance (d), etc.
2) Solution 1 calculates the kinetic energy of a 1000 lb satellite moving at 14,000 mi/h.
3) Solution 3 part b calculates the height a stone must be dropped from to achieve a kinetic energy of 576 J on the moon, given the stone's weight and acceleration of gravity are different on the moon.
JEE Physics/ Lakshmikanta Satapathy/ Simple harmonic motion QA part 6/ Question on amplitude of SHM determined from its total energy solved with the related concepts
Bound State Solution of the Klein–Gordon Equation for the Modified Screened C...BRNSS Publication Hub
We present solution of the Klein–Gordon equation for the modified screened Coulomb potential (Yukawa) plus inversely quadratic Yukawa potential through formula method. The conventional formula method which constitutes a simple formula for finding bound state solution of any quantum mechanical wave equation, which is simplified to the form; 2122233()()''()'()()0(1)(1)kksAsBscsssskssks−++ψ+ψ+ψ=−−. The bound state energy eigenvalues and its corresponding wave function obtained with its efficiency in spectroscopy.
Key words: Bound state, inversely quadratic Yukawa, Klein–Gordon, modified screened coulomb (Yukawa), quantum wave equation
The document describes three models of photons with physical extent beyond the traditional point particle model: a KdV particle, a normal probability classical packet, and a sinc function quantum packet. The sinc function model is identified as most suitable, describing a photon peaked at its origin that converges to ±∞. In this model, the photon has a disk shape with radii ranging from 10-17m for gamma rays to unlimited sizes for long radio wavelengths. The photon is proposed to have internal magnetic fields and a possible rest mass upper limit of 2×10-69kg.
EXACT SOLUTIONS OF SCHRÖDINGER EQUATION WITH SOLVABLE POTENTIALS FOR NON PT/P...ijrap
We have obtained explicitly the exact solutions of the Schrodinger equation with Non PT/PT symmetric
Rosen Morse II, Scarf II and Coulomb potentials. Energy eigenvalues and the corresponding
unnormalized wave functions for these systems for both Non PT and PT symmetric are also obtained using
the Nikiforov-Uvarov (NU) method.
The document summarizes problems involving calculating reaction forces at supports of structures using Lame's theorem and the principles of equilibrium. It provides 10 example problems showing the application of these principles to determine unknown reaction forces and loads. Diagrams accompany each problem showing the free body diagram and relevant forces and dimensions. Step-by-step solutions are provided for each problem applying the equations of equilibrium.
This document derives five equations that describe motion with constant acceleration. The first two equations are considered the most essential as the other three can be derived from combinations of the first two. Equation 1 relates the change in velocity to acceleration and time. Equation 2 relates the displacement to the initial velocity, acceleration, and time. The document shows the step-by-step work to derive each equation from fundamental kinematic equations and relationships between variables like average and instantaneous values.
The properties of neutrinos (the electric charge, the neutrino mass, rhe neutrino velocity, the oscillation of neutrinos) are obtained from the neutrino matricies representation.
1) The document contains solutions to physics problems involving kinetics energy (T), work (W), velocity (v), mass (m), distance (d), etc.
2) Solution 1 calculates the kinetic energy of a 1000 lb satellite moving at 14,000 mi/h.
3) Solution 3 part b calculates the height a stone must be dropped from to achieve a kinetic energy of 576 J on the moon, given the stone's weight and acceleration of gravity are different on the moon.
JEE Physics/ Lakshmikanta Satapathy/ Simple harmonic motion QA part 6/ Question on amplitude of SHM determined from its total energy solved with the related concepts
Bound State Solution of the Klein–Gordon Equation for the Modified Screened C...BRNSS Publication Hub
We present solution of the Klein–Gordon equation for the modified screened Coulomb potential (Yukawa) plus inversely quadratic Yukawa potential through formula method. The conventional formula method which constitutes a simple formula for finding bound state solution of any quantum mechanical wave equation, which is simplified to the form; 2122233()()''()'()()0(1)(1)kksAsBscsssskssks−++ψ+ψ+ψ=−−. The bound state energy eigenvalues and its corresponding wave function obtained with its efficiency in spectroscopy.
Key words: Bound state, inversely quadratic Yukawa, Klein–Gordon, modified screened coulomb (Yukawa), quantum wave equation
The document describes three models of photons with physical extent beyond the traditional point particle model: a KdV particle, a normal probability classical packet, and a sinc function quantum packet. The sinc function model is identified as most suitable, describing a photon peaked at its origin that converges to ±∞. In this model, the photon has a disk shape with radii ranging from 10-17m for gamma rays to unlimited sizes for long radio wavelengths. The photon is proposed to have internal magnetic fields and a possible rest mass upper limit of 2×10-69kg.
EXACT SOLUTIONS OF SCHRÖDINGER EQUATION WITH SOLVABLE POTENTIALS FOR NON PT/P...ijrap
We have obtained explicitly the exact solutions of the Schrodinger equation with Non PT/PT symmetric
Rosen Morse II, Scarf II and Coulomb potentials. Energy eigenvalues and the corresponding
unnormalized wave functions for these systems for both Non PT and PT symmetric are also obtained using
the Nikiforov-Uvarov (NU) method.
The document summarizes problems involving calculating reaction forces at supports of structures using Lame's theorem and the principles of equilibrium. It provides 10 example problems showing the application of these principles to determine unknown reaction forces and loads. Diagrams accompany each problem showing the free body diagram and relevant forces and dimensions. Step-by-step solutions are provided for each problem applying the equations of equilibrium.
This document derives five equations that describe motion with constant acceleration. The first two equations are considered the most essential as the other three can be derived from combinations of the first two. Equation 1 relates the change in velocity to acceleration and time. Equation 2 relates the displacement to the initial velocity, acceleration, and time. The document shows the step-by-step work to derive each equation from fundamental kinematic equations and relationships between variables like average and instantaneous values.
The properties of neutrinos (the electric charge, the neutrino mass, rhe neutrino velocity, the oscillation of neutrinos) are obtained from the neutrino matricies representation.
Bound- State Solution of Schrodinger Equation with Hulthen Plus Generalized E...ijrap
- The document discusses using the Nikiforov-Uvarov method to find bound state solutions to the Schrodinger equation with Hulthen plus generalized exponential Coulomb potential.
- The method is applied to obtain the energy eigenvalues and total wave function for the potential.
- A C++ algorithm is used to numerically calculate the energy values for different quantum states and screening parameter values.
Bound State Solution to Schrodinger Equation with Hulthen Plus Exponential Co...ijrap
In this work, we obtained an approximate bound state solution to Schrodinger with Hulthen plus
exponential Coulombic potential with centrifugal potential barrier using parametric Nikiforov-Uvarov
method. We obtained both the eigen energy and the wave functions to non -relativistic wave equations. We
implement Matlab algorithm to obtained the numerical bound state energies for various values of
adjustable screening parameter at various quantum state.. The developed potential reduces to Hulthen
potential and the numerical bound state energy conform to that of existing literature.
Numerical Methods and Analysis discusses various root-finding methods including bisection, false position, and Newton-Raphson. Bisection uses interval halving to find a root between two values with opposite signs. False position uses the slope of a line between two points to estimate the next root. Newton-Raphson approximates the root using Taylor series expansion neglecting higher order terms. Interpolation uses forward difference tables to construct a polynomial approximation of a function.
This document discusses the formulation of fractional supersymmetric theories in one dimension. It begins by presenting fractional superspace and fractional supersymmetry of order F=3, including the fractional supersymmetry transformations. It then derives the fractional supercharges and Euler-Lagrange equations for F=3. Finally, it generalizes the formulation to arbitrary fractional order F ≥ 3 by introducing fractional superspace and supersymmetry transformations of order F, as well as an action invariant under such transformations.
SOLUTIONS OF THE SCHRÖDINGER EQUATION WITH INVERSELY QUADRATIC HELLMANN PLUS ...ijrap
The solutions of the Schrödinger equation with inversely quadratic Hellmann plus Mie-type potential for
any angular momentum quantum number have been presented using the Nikiforov-Uvarov method. The
bound state energy eigenvalues and the corresponding un-normalized eigenfunctions are obtained in terms
of the Laguerre polynomials. Several cases of the potential are also considered and their eigen values obtained.
The document describes the flexibility method for analyzing statically indeterminate beams. It discusses:
- James Clerk Maxwell published the first treatment of the flexibility method in 1864, which was later extended by Otto Mohr.
- The method introduces compatibility equations involving displacements at redundant forces to provide additional equations for solving statically indeterminate structures.
- For a two-span beam example, the redundant reaction at the middle support is chosen, compatibility equations are written, and the flexibility matrix method is demonstrated to solve for redundant forces.
2d beam element with combined loading bending axial and torsionrro7560
The document discusses beam theory and finite element modeling of beams and frames. It provides information on modeling beams using one-dimensional beam elements with cubic shape functions. The formulation describes defining the element stiffness matrix and calculating the element's contribution to the global structural stiffness matrix and force vector based on applied loads. Boundary conditions and sample problems are presented to demonstrate the element modeling approach.
This document analyzes an indeterminate truss using the flexibility method. It first calculates the static degree of indeterminacy as 2. It then selects members OA and OD as redundant members. The truss is analyzed when each redundant member is given a force of 1 kN. A flexibility matrix equation is developed and solved to determine the redundant forces, which are then used to calculate the final forces in each member. The final forces show member OA in tension and member OD in compression.
1) The motion of an electric dipole in a magnetic field is coupled between translation and rotation. The conservation laws for momentum and angular momentum are modified.
2) For a dipole of two charges connected by a rigid rod, the conserved quantities are the total momentum P and energy E, which are functions of the center of mass velocity and angular velocity.
3) The quantity J, defined as the sum of the cross product of the center of mass position and total momentum with the angular momentum, is also conserved.
ANALYTICAL SOLUTIONS OF THE MODIFIED COULOMB POTENTIAL USING THE FACTORIZATIO...ijrap
This document presents analytical solutions to the Schrödinger equation with a modified Coulomb potential using the factorization method. The energy levels and wave functions are obtained in terms of associated Laguerre polynomials. Energy eigenvalues are computed for selected elements like hydrogen, lithium, sodium, potassium and copper for various values of n and l. The results show the expected degeneracies and reduce to the Coulomb energy solution when appropriate limits are taken.
This document presents theoretical problems related to ionic crystal structures. It discusses the Coulomb and repulsive potentials acting on ions in the crystal lattice. Two models are provided to describe the repulsive potential: an exponential function and an inverse power function. Experimental data for several ionic crystals is given. The problems involve deriving expressions for the net potential energy, determining equilibrium positions, estimating potential parameters from experimental dissociation energies, and calculating ionization energies. The solutions show that the Coulomb and Pauli potentials contribute to the net potential energy in a 9:1 proportion for NaCl.
The document summarizes key points from Physics 111 Lecture 2:
1) It recaps 1-D constant acceleration motion and introduces 1-D free fall, reviewing that gravity causes a downward acceleration.
2) Vectors in 2D and 3D are discussed, including vector addition and unit vectors.
3) Kinematics equations for constant acceleration are extended to 3D motion, and it is noted that for constant acceleration, most 3D problems can be reduced to 2D.
4) Examples of projectile motion and 2D motion are presented to demonstrate applying the concepts.
- The document provides the solution to problem 25.72 from the textbook, which asks to derive an expression for the total electric potential energy of a solid sphere with uniform charge density.
- The sphere is modeled as being built up of concentric spherical shells, with each shell carrying a small charge dq.
- The expression derived for the total potential energy is Ue = (3/5)kεQ2/R, where Q is the total charge on the sphere, R is the radius, and kε is the Coulomb's constant.
- The derivation involves integrating the electric potential energy dUe = Vdq over the volume of the sphere, where V is the potential and dq is the charge
This document summarizes information from a textbook chapter on elementary particles and the beginning of the universe. It provides examples of how to identify unknown particles in decay reactions using conservation laws of charge number, baryon number, strangeness, and spin. It also gives possible quark combinations for specific baryon particles. One example calculates the distance to a galaxy receding from Earth at 2.5% the speed of light using Hubble's law.
It is a algorithm used to find a minimum cost spanning tree for connected weighted undirected graph.This algorithm first appeared in Proceedings of the American Mathematical Society in 1956, and was written by Joseph Kruskal.
Ibiza is a small island that is looking forward to welcoming visitors. The island's teachers are excited for people to come experience Ibiza. In a nutshell, this document provides a brief introduction about Ibiza and expresses that both the island's residents and educators are eager for others to visit.
In this file, you can ref useful information about performance management and appraisal such as performance management and appraisal methods, performance management and appraisal tips, performance management and appraisal forms, performance management and appraisal phrases … If you need more assistant for performance management and appraisal, please leave your comment at the end of file.
Bound- State Solution of Schrodinger Equation with Hulthen Plus Generalized E...ijrap
- The document discusses using the Nikiforov-Uvarov method to find bound state solutions to the Schrodinger equation with Hulthen plus generalized exponential Coulomb potential.
- The method is applied to obtain the energy eigenvalues and total wave function for the potential.
- A C++ algorithm is used to numerically calculate the energy values for different quantum states and screening parameter values.
Bound State Solution to Schrodinger Equation with Hulthen Plus Exponential Co...ijrap
In this work, we obtained an approximate bound state solution to Schrodinger with Hulthen plus
exponential Coulombic potential with centrifugal potential barrier using parametric Nikiforov-Uvarov
method. We obtained both the eigen energy and the wave functions to non -relativistic wave equations. We
implement Matlab algorithm to obtained the numerical bound state energies for various values of
adjustable screening parameter at various quantum state.. The developed potential reduces to Hulthen
potential and the numerical bound state energy conform to that of existing literature.
Numerical Methods and Analysis discusses various root-finding methods including bisection, false position, and Newton-Raphson. Bisection uses interval halving to find a root between two values with opposite signs. False position uses the slope of a line between two points to estimate the next root. Newton-Raphson approximates the root using Taylor series expansion neglecting higher order terms. Interpolation uses forward difference tables to construct a polynomial approximation of a function.
This document discusses the formulation of fractional supersymmetric theories in one dimension. It begins by presenting fractional superspace and fractional supersymmetry of order F=3, including the fractional supersymmetry transformations. It then derives the fractional supercharges and Euler-Lagrange equations for F=3. Finally, it generalizes the formulation to arbitrary fractional order F ≥ 3 by introducing fractional superspace and supersymmetry transformations of order F, as well as an action invariant under such transformations.
SOLUTIONS OF THE SCHRÖDINGER EQUATION WITH INVERSELY QUADRATIC HELLMANN PLUS ...ijrap
The solutions of the Schrödinger equation with inversely quadratic Hellmann plus Mie-type potential for
any angular momentum quantum number have been presented using the Nikiforov-Uvarov method. The
bound state energy eigenvalues and the corresponding un-normalized eigenfunctions are obtained in terms
of the Laguerre polynomials. Several cases of the potential are also considered and their eigen values obtained.
The document describes the flexibility method for analyzing statically indeterminate beams. It discusses:
- James Clerk Maxwell published the first treatment of the flexibility method in 1864, which was later extended by Otto Mohr.
- The method introduces compatibility equations involving displacements at redundant forces to provide additional equations for solving statically indeterminate structures.
- For a two-span beam example, the redundant reaction at the middle support is chosen, compatibility equations are written, and the flexibility matrix method is demonstrated to solve for redundant forces.
2d beam element with combined loading bending axial and torsionrro7560
The document discusses beam theory and finite element modeling of beams and frames. It provides information on modeling beams using one-dimensional beam elements with cubic shape functions. The formulation describes defining the element stiffness matrix and calculating the element's contribution to the global structural stiffness matrix and force vector based on applied loads. Boundary conditions and sample problems are presented to demonstrate the element modeling approach.
This document analyzes an indeterminate truss using the flexibility method. It first calculates the static degree of indeterminacy as 2. It then selects members OA and OD as redundant members. The truss is analyzed when each redundant member is given a force of 1 kN. A flexibility matrix equation is developed and solved to determine the redundant forces, which are then used to calculate the final forces in each member. The final forces show member OA in tension and member OD in compression.
1) The motion of an electric dipole in a magnetic field is coupled between translation and rotation. The conservation laws for momentum and angular momentum are modified.
2) For a dipole of two charges connected by a rigid rod, the conserved quantities are the total momentum P and energy E, which are functions of the center of mass velocity and angular velocity.
3) The quantity J, defined as the sum of the cross product of the center of mass position and total momentum with the angular momentum, is also conserved.
ANALYTICAL SOLUTIONS OF THE MODIFIED COULOMB POTENTIAL USING THE FACTORIZATIO...ijrap
This document presents analytical solutions to the Schrödinger equation with a modified Coulomb potential using the factorization method. The energy levels and wave functions are obtained in terms of associated Laguerre polynomials. Energy eigenvalues are computed for selected elements like hydrogen, lithium, sodium, potassium and copper for various values of n and l. The results show the expected degeneracies and reduce to the Coulomb energy solution when appropriate limits are taken.
This document presents theoretical problems related to ionic crystal structures. It discusses the Coulomb and repulsive potentials acting on ions in the crystal lattice. Two models are provided to describe the repulsive potential: an exponential function and an inverse power function. Experimental data for several ionic crystals is given. The problems involve deriving expressions for the net potential energy, determining equilibrium positions, estimating potential parameters from experimental dissociation energies, and calculating ionization energies. The solutions show that the Coulomb and Pauli potentials contribute to the net potential energy in a 9:1 proportion for NaCl.
The document summarizes key points from Physics 111 Lecture 2:
1) It recaps 1-D constant acceleration motion and introduces 1-D free fall, reviewing that gravity causes a downward acceleration.
2) Vectors in 2D and 3D are discussed, including vector addition and unit vectors.
3) Kinematics equations for constant acceleration are extended to 3D motion, and it is noted that for constant acceleration, most 3D problems can be reduced to 2D.
4) Examples of projectile motion and 2D motion are presented to demonstrate applying the concepts.
- The document provides the solution to problem 25.72 from the textbook, which asks to derive an expression for the total electric potential energy of a solid sphere with uniform charge density.
- The sphere is modeled as being built up of concentric spherical shells, with each shell carrying a small charge dq.
- The expression derived for the total potential energy is Ue = (3/5)kεQ2/R, where Q is the total charge on the sphere, R is the radius, and kε is the Coulomb's constant.
- The derivation involves integrating the electric potential energy dUe = Vdq over the volume of the sphere, where V is the potential and dq is the charge
This document summarizes information from a textbook chapter on elementary particles and the beginning of the universe. It provides examples of how to identify unknown particles in decay reactions using conservation laws of charge number, baryon number, strangeness, and spin. It also gives possible quark combinations for specific baryon particles. One example calculates the distance to a galaxy receding from Earth at 2.5% the speed of light using Hubble's law.
It is a algorithm used to find a minimum cost spanning tree for connected weighted undirected graph.This algorithm first appeared in Proceedings of the American Mathematical Society in 1956, and was written by Joseph Kruskal.
Ibiza is a small island that is looking forward to welcoming visitors. The island's teachers are excited for people to come experience Ibiza. In a nutshell, this document provides a brief introduction about Ibiza and expresses that both the island's residents and educators are eager for others to visit.
In this file, you can ref useful information about performance management and appraisal such as performance management and appraisal methods, performance management and appraisal tips, performance management and appraisal forms, performance management and appraisal phrases … If you need more assistant for performance management and appraisal, please leave your comment at the end of file.
In this file, you can ref useful information about employee performance appraisal such as employee performance appraisal methods, employee performance appraisal tips, employee performance appraisal forms, employee performance appraisal phrases … If you need more assistant for employee performance appraisal, please leave your comment at the end of file.
The document summarizes the applicant's experience as a safety professional on industrial construction projects over the past 5 years. He is seeking a new position as a safety representative in Northern Utah and lists relevant experience ensuring safety compliance and training workers on safety policies and procedures at oil refineries and industrial sites.
This document provides a summary of George Nabil Basalious's personal and professional details. It includes his contact information, education history, skills, work experience, and references. He has a B.Sc. in Civil Engineering from El Fayoum University in Egypt and over 5 years of work experience as a site engineer and building department manager assistant on projects like ERC Refinery Project, Mall of Egypt, and BYOUM RESIDENCE. His skills include languages of Arabic and English, AutoCAD, project management, engineering courses, and summer training at ORASCOM Construction Industries.
1. The author teaches English literature at the University of Human Development in Iraqi Kurdistan. His students are not typically what Westerners imagine - heroic guerilla fighters bringing guns to class. Instead, they are generous, spirited people who are vocal advocates for feminism, democracy, and human rights.
2. Kurdish students are accustomed to a rote learning style in their previous schooling that discourages individual thought. They are excited by the opportunity for self-expression and debate in university but sometimes struggle with more abstract critical thinking. The author works to develop their analytical skills over time.
3. Kurdish students are naturally collaborative and responsive to literature, easily identifying with characters and their suffering. While
In this file, you can ref useful information about importance of performance appraisal such as importance of performance appraisal methods, importance of performance appraisal tips, importance of performance appraisal forms, importance of performance appraisal phrases … If you need more assistant for importance of performance appraisal, please leave your comment at the end of file.
Este documento presenta la programación musical que se tocará en Puig d'en Valls durante varios meses. La programación incluye bandas sonoras, musicales, rock, pop, ritmos latinos y canciones navideñas y de carnaval. La programación podría variar según las solicitudes de los estudiantes.
Tendencias en un Service Desk (Jornadas de Excelencia Virtuales ITSM (JEVi) 2...Gabriel Martínez Martínez
La ponencia quiere servir de base para identificar qué tendencias pueden formar parte de un plan director de un Service Desk (SD).
En función de los objetivos de un SD, el responsable del mismo puede identificar cuáles de las tendencias pueden aplicar, y dónde y qué valor pueden generar, de cara a definir el Plan Director de su SD.
El documento describe los principios y valores fundamentales del cooperativismo. El cooperativismo promueve la organización de personas para satisfacer sus necesidades de manera conjunta. Los siete principios cooperativos incluyen la adhesión voluntaria, el control democrático, la participación económica, la autonomía e independencia, la educación, la cooperación entre cooperativas y el interés por la comunidad. Los valores centrales son la ayuda mutua, la responsabilidad propia, la democracia, la igualdad y la solidaridad.
Iit jam 2016 physics solutions BY TrajectoryeducationDev Singh
1. The electric field at a point (a, b, 0) due to an infinitely long wire with uniform line charge density λ is given by E=λ/(2πε0)(a/r2)ex+(b/r2)ey, where r2=a2+b2.
2. For a 1W point source emitting light uniformly in all directions, the Poynting vector at the point (1, 1, 0) is 1/(8π)ex+(y/e)ey W/cm2.
3. A charged particle starting from the origin with velocity 3/2ex+2ez m/s in a uniform magnetic field B=B
This document provides an overview of structural dynamics and free vibration analysis of single degree of freedom systems. It defines key concepts like natural frequency, damping, and logarithmic decrement. Methods for analyzing undamped and damped free vibration are presented. Examples show how to calculate the natural frequency, time period, amplitude, and displacement as a function of time for undamped systems subjected to initial displacement or velocity conditions. Analysis of damped systems models the response as a decaying exponential function.
This document provides an overview of structural dynamics and free vibration analysis of single degree of freedom (SDOF) systems. It defines key terms like natural frequency, damping, and logarithmic decrement. Methods are presented for analyzing the free vibration of undamped and damped SDOF systems under initial displacement conditions. Examples are provided to demonstrate calculating the natural frequency, time period, amplitude, and displacement over time of vibrating SDOF structures.
The document describes a study that investigated the effect of using computer simulations in teaching physics concepts related to oscillations at the undergraduate level. The study aimed to identify difficulties students face in learning oscillations, develop a computer simulation package and assessment tool, and measure the impact of the simulations compared to traditional teaching methods. Results showed that students who used the simulations had significantly higher normalized learning gains compared to the control group on a post-test of oscillations concepts.
The document discusses the results of an exam in a physics class on elasticity and oscillations. It provides the grade distributions and averages for the exam, along with lecture materials on springs, Hooke's law, simple harmonic motion, and examples of physics problems involving springs and oscillations. Key concepts covered include restoring forces, potential energy in springs, Young's modulus, and the equations of motion for simple harmonic oscillators.
The document discusses the results of an exam in a physics class on elasticity and oscillations. It provides the grade distributions and averages for the exam, along with lecture materials on springs, Hooke's law, simple harmonic motion, and examples of physics problems involving springs and oscillations. Key concepts covered include restoring forces, potential energy in springs, Young's modulus, and the equations of motion for simple harmonic oscillators.
This document provides detailed solutions to the 2013 JEE Advanced Paper 1 with code 0. It contains solutions to 10 multiple choice questions in Section 1 and 5 multiple choice questions in Section 2 of the Physics portion of the exam. The solutions explain the conceptual reasoning and calculations for arriving at the correct answers. Key details provided in the solutions include relevant equations, diagrams, and step-by-step working.
The document discusses dynamic modeling of robot manipulators using the Euler-Lagrange approach. It introduces dynamic models and the direct and inverse problems. The Euler-Lagrange approach is then explained in detail. It involves computing the kinetic and potential energies of each link based on the link masses, centers of mass, moments of inertia, and joint velocities and positions. This allows deriving the dynamic equations of motion for the manipulator.
This document contains information about JEE Advanced 2015 Paper 2 Code 3 for Physics. It includes 10 multiple choice questions testing concepts in physics. The questions cover topics such as optics, circuits, quantum mechanics, mechanics, thermodynamics and electromagnetism. For each question, students had to select the single correct answer ranging from 0 to 9. The document also provides two additional sections with more complex multi-concept questions, some requiring selecting one or more answers. The questions test a range of fundamental physics principles and problem solving abilities.
This document contains 20 questions related to quantum chemistry and elementary quantum mechanical models. The questions cover topics like calculating the momentum, velocity and de Broglie wavelength of an electron; estimating the kinetic energy of an electron in a particle in a box model; obtaining the energy eigenfunctions and eigenvalues for particles in one-dimensional boxes; and commutators of operators. The document tests understanding of fundamental quantum mechanical concepts like the particle in a box model, energy eigenfunctions, eigenvalues, normalization, and commutators.
Solution to schrodinger equation with dirac comb potential slides
This document summarizes solving the Schrödinger equation for a Dirac comb potential. The potential is an infinite series of Dirac delta functions spaced periodically. Floquet theory is used to solve the time-independent Schrödinger equation for this potential. Boundary conditions are applied and the resulting equations are solved graphically. Allowed energy bands are determined and plotted versus wave vector for both attractive and repulsive delta function potentials.
The document contains multiple conceptual physics problems involving conservation of energy.
1) A system of two cylinders connected by a cord over a frictionless peg is released from rest. The system's mechanical energy is conserved, so the potential energy decreases and kinetic energy increases.
2) Estimation problems calculate the minimum time to climb stairs or the Empire State Building using assumptions about maximum metabolic rate and efficiency.
3) Multiple other problems apply conservation of mechanical energy to calculate quantities like tension, equilibrium angles, or speeds in various physical systems like swings or circular motion.
Jee advanced 2015 paper 1 code 1 final Pradeep Kumar
1. The document provides information about JEE Advanced 2015 paper 1, including 8 multiple choice questions in Section 1 and 10 multiple choice questions in Section 2.
2. Section 3 contains 2 matching questions matching concepts in Column I to statements in Column II.
3. The questions cover topics in physics including electromagnetism, quantum mechanics, thermodynamics, and nuclear physics.
This document contains instructions and problems related to a physics exam on relativistic particles and superconducting magnets. It includes 4 problems:
1) Describing the motion of a relativistic particle subject to an attractive central force, including graphs of position vs time and momentum vs position.
2) Modeling a meson as two quarks with a central attractive force, and graphing their motion.
3) Transforming the motion graphs from problem 2 into a different reference frame moving at 0.6c.
4) Calculating the energy of a meson moving at 0.6c as observed in the lab frame.
The document provides answer sheets for the problems and specifies the
The document provides information about potential energy curves and conservative forces:
1) It gives an example problem about calculating the speed and turning point of a particle moving in one-dimensional motion based on its potential energy curve.
2) It discusses how to calculate the force acting on a particle using the slope of the potential energy curve.
3) It covers concepts like work done by external forces, changes in mechanical and thermal energy, and how potential energy and kinetic energy relate for conservative systems.
Neet full syllabus test paper physics chemistry biologypravallikadodda
This document describes a 35 question physics exam with the following details:
- Section 1 is mandatory and contains 35 questions worth 4 marks each for correct answers and a 1 mark deduction for incorrect answers.
- Section 2 also contains physics questions, with 10 of 15 questions being mandatory with the same scoring scheme as Section 1.
- The questions cover various topics in physics including mechanics, waves, optics, thermodynamics and electromagnetism. Sample questions on momentum, simple harmonic motion, wave interference and gas laws are provided.
- Students must select the correct answer from the multiple choice options provided for each question.
The document discusses static analysis methods for laminated composite plates using energy methods. It describes the principle of total potential energy and how to apply it to analyze laminated plates. As an example, it analyzes a simply supported rectangular plate under a uniform load using both classical and energy methods, showing the energy method provides more accurate results when bending-twisting coupling is present.
(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.
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.
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.
JAMES WEBB STUDY THE MASSIVE BLACK HOLE SEEDSSérgio Sacani
The pathway(s) to seeding the massive black holes (MBHs) that exist at the heart of galaxies in the present and distant Universe remains an unsolved problem. Here we categorise, describe and quantitatively discuss the formation pathways of both light and heavy seeds. We emphasise that the most recent computational models suggest that rather than a bimodal-like mass spectrum between light and heavy seeds with light at one end and heavy at the other that instead a continuum exists. Light seeds being more ubiquitous and the heavier seeds becoming less and less abundant due the rarer environmental conditions required for their formation. We therefore examine the different mechanisms that give rise to different seed mass spectrums. We show how and why the mechanisms that produce the heaviest seeds are also among the rarest events in the Universe and are hence extremely unlikely to be the seeds for the vast majority of the MBH population. We quantify, within the limits of the current large uncertainties in the seeding processes, the expected number densities of the seed mass spectrum. We argue that light seeds must be at least 103 to 105 times more numerous than heavy seeds to explain the MBH population as a whole. Based on our current understanding of the seed population this makes heavy seeds (Mseed > 103 M⊙) a significantly more likely pathway given that heavy seeds have an abundance pattern than is close to and likely in excess of 10−4 compared to light seeds. Finally, we examine the current state-of-the-art in numerical calculations and recent observations and plot a path forward for near-future advances in both domains.
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!
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.
Immersive Learning That Works: Research Grounding and Paths ForwardLeonel Morgado
We will metaverse into the essence of immersive learning, into its three dimensions and conceptual models. This approach encompasses elements from teaching methodologies to social involvement, through organizational concerns and technologies. Challenging the perception of learning as knowledge transfer, we introduce a 'Uses, Practices & Strategies' model operationalized by the 'Immersive Learning Brain' and ‘Immersion Cube’ frameworks. This approach offers a comprehensive guide through the intricacies of immersive educational experiences and spotlighting research frontiers, along the immersion dimensions of system, narrative, and agency. Our discourse extends to stakeholders beyond the academic sphere, addressing the interests of technologists, instructional designers, and policymakers. We span various contexts, from formal education to organizational transformation to the new horizon of an AI-pervasive society. This keynote aims to unite the iLRN community in a collaborative journey towards a future where immersive learning research and practice coalesce, paving the way for innovative educational research and practice landscapes.
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.
Candidate young stellar objects in the S-cluster: Kinematic analysis of a sub...Sérgio Sacani
Context. The observation of several L-band emission sources in the S cluster has led to a rich discussion of their nature. However, a definitive answer to the classification of the dusty objects requires an explanation for the detection of compact Doppler-shifted Brγ emission. The ionized hydrogen in combination with the observation of mid-infrared L-band continuum emission suggests that most of these sources are embedded in a dusty envelope. These embedded sources are part of the S-cluster, and their relationship to the S-stars is still under debate. To date, the question of the origin of these two populations has been vague, although all explanations favor migration processes for the individual cluster members. Aims. This work revisits the S-cluster and its dusty members orbiting the supermassive black hole SgrA* on bound Keplerian orbits from a kinematic perspective. The aim is to explore the Keplerian parameters for patterns that might imply a nonrandom distribution of the sample. Additionally, various analytical aspects are considered to address the nature of the dusty sources. Methods. Based on the photometric analysis, we estimated the individual H−K and K−L colors for the source sample and compared the results to known cluster members. The classification revealed a noticeable contrast between the S-stars and the dusty sources. To fit the flux-density distribution, we utilized the radiative transfer code HYPERION and implemented a young stellar object Class I model. We obtained the position angle from the Keplerian fit results; additionally, we analyzed the distribution of the inclinations and the longitudes of the ascending node. Results. The colors of the dusty sources suggest a stellar nature consistent with the spectral energy distribution in the near and midinfrared domains. Furthermore, the evaporation timescales of dusty and gaseous clumps in the vicinity of SgrA* are much shorter ( 2yr) than the epochs covered by the observations (≈15yr). In addition to the strong evidence for the stellar classification of the D-sources, we also find a clear disk-like pattern following the arrangements of S-stars proposed in the literature. Furthermore, we find a global intrinsic inclination for all dusty sources of 60 ± 20◦, implying a common formation process. Conclusions. The pattern of the dusty sources manifested in the distribution of the position angles, inclinations, and longitudes of the ascending node strongly suggests two different scenarios: the main-sequence stars and the dusty stellar S-cluster sources share a common formation history or migrated with a similar formation channel in the vicinity of SgrA*. Alternatively, the gravitational influence of SgrA* in combination with a massive perturber, such as a putative intermediate mass black hole in the IRS 13 cluster, forces the dusty objects and S-stars to follow a particular orbital arrangement. Key words. stars: black holes– stars: formation– Galaxy: center– galaxies: star formation
1. Physics 101 Learning Object 1:
Energy Conservation in Simple Harmonic Motion
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Image gathered from: http://homepages.spa.umn.edu/~yk/Image28.gif
!
!
The above diagram shows 5 different mass-spring systems at different X
distances, with all blocks with the same mass of 4kg.
!
!
Question 1. In system (a), if distance X is -6cm, what is the total energy at that
point? Choose the answer given in terms of k (constant) and v (velocity).
A. 0 J
B. 3k J
C. 18k J
D. -18k J
E. 18k + 2v2
!
Question 2. In system (c), with the distance of X=0cm, what is the total energy
at that point? Choose the answer given in terms of k (constant) and v (velocity).
!
A. 0 J
B. 2v2
J
C. 4kv2
J
D. 4v2
J
E. 8v2
J
!
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2. Question 3. In system (d), when X=4cm, what is the total energy in terms of k
(constant) and v (velocity)?
!
A. 8k J
B. 16k J
C. 4v2
- 8k J
D. 2v2
- 8k J
E. 2v2
+ 8k J
!
Question 4. In system (e), when X=6cm, what is the total energy in terms of k
(constant) and v (velocity)?
!
A. 36k J
B. 18k J
C. -18k J
D. 18k + 2v2
J
E. 36k + 2v2
J
!
Question 5. In all 5 of the systems, which system contains the most total
energy?
!
A. All systems have the same total energy.
B. (c)
C. (e)
D. (a)
E. Impossible to determine without more information.
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3. Physics 101 Learning Object 1:
Energy Conservation in Simple Harmonic Motion
!
Image gathered from: http://homepages.spa.umn.edu/~yk/Image28.gif
!
!
The above diagram shows 5 different mass-spring systems at different X
distances, with all blocks with the same mass of 4kg.
!
!
Question 1. In system (a), if distance X is -6cm, what is the total energy at that
point? Choose the answer given in terms of k (constant) and v (velocity).
A. 0 J
B. 3k J
C. 18k J
D. -18k J
E. 18k + 2v2
!
Answer: C. Since total energy (X=-6, v=0) = K + U = (1/2)kX2
= (1/2)(-6)2
k =
18k J
!
Question 2. In system (c), with the distance of X=0cm, what is the total energy
at that point? Choose the answer given in terms of k (constant) and v (velocity).
!
A. 0 J
B. 2v2
J
C. 4kv2
J
Page of3 4
4. D. 4v2
J
E. 8v2
J
!
Answer: B. Total energy (X=0) = K + U = (1/2)mv2
= (1/2)(4)v2
= 2v2
J
!
Question 3. In system (d), when X=4cm, what is the total energy in terms of k
(constant) and v (velocity)?
!
A. 8k J
B. 16k J
C. 4v2
- 8k J
D. 2v2
- 8k J
E. 2v2
+ 8k J
!
Answer: E. Total energy (X=4) = K + U = (1/2)mv2
+ (1/2)kX2
= (1/2)(4)v2
+
(1/2)(4)2
k = 2v2
+ 8k J
!
Question 4. In system (e), when X=6cm, what is the total energy in terms of k
(constant) and v (velocity)?
!
A. 36k J
B. 18k J
C. -18k J
D. 18k + 2v2
J
E. 36k + 2v2
J
!
Answer: B. Total energy (X=6, v=0) = K + U = (1/2)kX2
= (1/2)(6)2
k = 18k J
!
Question 5. In all 5 of the systems, which system contains the most total
energy?
!
A. All systems have the same total energy.
B. (c)
C. (e)
D. (a)
E. Impossible to determine without more information.
Answer: A. Due to the conservation of energy, all systems will have the same
total energy with the formula E = K + U.
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