The presentation opens up by introducing Schrodinger's time dependent and independent wave equation. Then it covers the derivation of time independent wave equation, followed by its applications.
Schrodinger equation and its applications: Chapter 2Dr.Pankaj Khirade
Wave function and its physical significance, Schrodinger time dependent equation, Separation in time dependent and time independent parts, Operators in quantum Mechanics, Eigen functions and Eigen values, Particle in one dimensional and three dimensional box (Energy eigen values). Qualitative analysis of potential barrier Tunneling effect). Simple Harmonic Oscillator (Qualitative analysis of Zero point energy)
This document discusses the uncertainty principle as stated by Werner Heisenberg in 1927. It provides Heisenberg's background and contributions to physics. The principle states that the momentum and position of a particle cannot be simultaneously measured with perfect precision due to inherent uncertainties. There is a minimum for the product of the uncertainties in these two measurements. The document explains this concept and provides the formula for the uncertainty principle.
1) The time-independent Schrodinger wave equation describes a standing wave with wavelength λ that has an amplitude at any point along the x direction.
2) In three dimensions, the Schrodinger wave equation incorporates second derivatives with respect to x, y, and z coordinates.
3) The Hamiltonian operator Ĥ in the time-independent Schrodinger wave equation is the Laplacian operator ∇2 plus 8π2m/h2 times the potential energy V.
The Schrodinger equation plays the role of Newton's laws and conservation of energy in classical mechanics by predicting the future behavior of dynamic systems. It is a wave equation that uses the wavefunction to analytically and precisely predict the probability of events or outcomes, though not the strict determination of a detailed outcome. The kinetic and potential energies are transformed into the Hamiltonian which acts on the wavefunction to generate its evolution in time and space, giving the quantized energies of the system and the form of the wavefunction to calculate other properties.
1. The document discusses the Fermi-Dirac distribution function, which describes the occupancy of energy levels by electrons in a solid.
2. The probability that an energy level E is filled by an electron is given by the Fermi-Dirac distribution function f(E) = 1/(1+e^(E-EF)/kT), where EF is the Fermi level energy.
3. The derivation of the Fermi-Dirac distribution function maximizes the logarithm of the multiplicity function, or number of configurations that electrons can occupy energy states, to find the occupancy probability that corresponds to thermal equilibrium.
Introduction to quantum mechanics and schrodinger equationGaurav Singh Gusain
Classical mechanics describes macroscopic objects while quantum mechanics describes microscopic objects due to limitations of classical theory. Quantum mechanics was introduced after classical mechanics failed to explain experimental observations involving microscopic particles. Some key aspects of quantum mechanics are the photoelectric effect, blackbody radiation, Compton effect, wave-particle duality, the Heisenberg uncertainty principle, and Schrodinger's wave equation. Schrodinger's equation describes the wave function and probability of finding a particle.
Lecture 8: Introduction to Quantum Chemical Simulation graduate course taught at MIT in Fall 2014 by Heather Kulik. This course covers: wavefunction theory, density functional theory, force fields and molecular dynamics and sampling.
Introduction to perturbation theory, part-1Kiran Padhy
Perturbation theory provides an approximate method for solving quantum mechanical problems where the Hamiltonian cannot be solved exactly. It involves splitting the Hamiltonian into an exactly solvable unperturbed part (H0) and a perturbed part (H1) treated as a small disturbance. The eigenvalues and eigenstates of the full Hamiltonian are expressed as power series expansions in terms of the perturbation strength parameter λ, allowing the effects of the perturbation to be calculated order by order. There are two types of perturbation theory: time-independent, where the unperturbed eigenstates are stationary; and time-dependent, where they vary with time under the perturbation.
Schrodinger equation and its applications: Chapter 2Dr.Pankaj Khirade
Wave function and its physical significance, Schrodinger time dependent equation, Separation in time dependent and time independent parts, Operators in quantum Mechanics, Eigen functions and Eigen values, Particle in one dimensional and three dimensional box (Energy eigen values). Qualitative analysis of potential barrier Tunneling effect). Simple Harmonic Oscillator (Qualitative analysis of Zero point energy)
This document discusses the uncertainty principle as stated by Werner Heisenberg in 1927. It provides Heisenberg's background and contributions to physics. The principle states that the momentum and position of a particle cannot be simultaneously measured with perfect precision due to inherent uncertainties. There is a minimum for the product of the uncertainties in these two measurements. The document explains this concept and provides the formula for the uncertainty principle.
1) The time-independent Schrodinger wave equation describes a standing wave with wavelength λ that has an amplitude at any point along the x direction.
2) In three dimensions, the Schrodinger wave equation incorporates second derivatives with respect to x, y, and z coordinates.
3) The Hamiltonian operator Ĥ in the time-independent Schrodinger wave equation is the Laplacian operator ∇2 plus 8π2m/h2 times the potential energy V.
The Schrodinger equation plays the role of Newton's laws and conservation of energy in classical mechanics by predicting the future behavior of dynamic systems. It is a wave equation that uses the wavefunction to analytically and precisely predict the probability of events or outcomes, though not the strict determination of a detailed outcome. The kinetic and potential energies are transformed into the Hamiltonian which acts on the wavefunction to generate its evolution in time and space, giving the quantized energies of the system and the form of the wavefunction to calculate other properties.
1. The document discusses the Fermi-Dirac distribution function, which describes the occupancy of energy levels by electrons in a solid.
2. The probability that an energy level E is filled by an electron is given by the Fermi-Dirac distribution function f(E) = 1/(1+e^(E-EF)/kT), where EF is the Fermi level energy.
3. The derivation of the Fermi-Dirac distribution function maximizes the logarithm of the multiplicity function, or number of configurations that electrons can occupy energy states, to find the occupancy probability that corresponds to thermal equilibrium.
Introduction to quantum mechanics and schrodinger equationGaurav Singh Gusain
Classical mechanics describes macroscopic objects while quantum mechanics describes microscopic objects due to limitations of classical theory. Quantum mechanics was introduced after classical mechanics failed to explain experimental observations involving microscopic particles. Some key aspects of quantum mechanics are the photoelectric effect, blackbody radiation, Compton effect, wave-particle duality, the Heisenberg uncertainty principle, and Schrodinger's wave equation. Schrodinger's equation describes the wave function and probability of finding a particle.
Lecture 8: Introduction to Quantum Chemical Simulation graduate course taught at MIT in Fall 2014 by Heather Kulik. This course covers: wavefunction theory, density functional theory, force fields and molecular dynamics and sampling.
Introduction to perturbation theory, part-1Kiran Padhy
Perturbation theory provides an approximate method for solving quantum mechanical problems where the Hamiltonian cannot be solved exactly. It involves splitting the Hamiltonian into an exactly solvable unperturbed part (H0) and a perturbed part (H1) treated as a small disturbance. The eigenvalues and eigenstates of the full Hamiltonian are expressed as power series expansions in terms of the perturbation strength parameter λ, allowing the effects of the perturbation to be calculated order by order. There are two types of perturbation theory: time-independent, where the unperturbed eigenstates are stationary; and time-dependent, where they vary with time under the perturbation.
This document introduces the Fermi-Dirac distribution function. It begins by discussing basic concepts like the Fermi level and Fermi energy. It then covers Fermi and Bose statistics, and the postulates of Fermi particles. The derivation of the Fermi-Dirac distribution function is shown, which gives the probability of a quantum state being occupied at a given energy and temperature. Graphs are presented showing how the distribution varies with different temperatures. The classical limit of the distribution is discussed. References are provided at the end.
1. Quantum mechanics began with Max Planck's paper in 1900 explaining black body radiation. It extends physics to small dimensions and includes classical laws as special cases.
2. Photoelectric effect shows that light behaves as particles called photons. Einstein's equation explained it using the photon energy.
3. Compton scattering showed that photons can collide with and transfer energy to electrons. The Compton wavelength was derived from this.
Nuclear Quadrupole Resonance Spectroscopy (NQR) is a chemical analysis technique that detects nuclear energy level transitions in the absence of a magnetic field through the absorption of radio frequency radiation. NQR is applicable to solids due to the quadrupole moment averaging to zero in liquids and gases. The interaction between a nucleus's quadrupole moment and the electric field gradient of its surroundings results in quantized energy levels. Transitions between these levels are detected as NQR spectra and provide information about electronic structure, hybridization, and charge distribution. NQR finds applications in studying charge transfer complexes, detecting crystal imperfections, and locating land mines.
Time Independent Perturbation Theory, 1st order correction, 2nd order correctionJames Salveo Olarve
The presentation is about how to solve the new energy levels and wave functions when the simple Hamiltonian is added by another term due to external effect (can be due to external field) .
The intended reader of this presentation were physics students. The author already assumed that the reader knows dirac braket notation.
This presentation shows a technique of how to solve for the approximate ground state energy using Schrodinger Equation in which the solution for wave function is not on hand
CHAPTER 6 Quantum Mechanics II
6.0 Partial differentials
6.1 The Schrödinger Wave Equation
6.2 Expectation Values
6.3 Infinite Square-Well Potential
6.4 Finite Square-Well Potential
6.5 Three-Dimensional Infinite-Potential Well
6.6 Simple Harmonic Oscillator
6.7 Barriers and Tunneling in some books an extra chapter due to its technical importance
The document discusses first order perturbation theory. It begins by introducing perturbation theory as an approximate method to solve the Schrodinger equation for complex quantum systems where the Hamiltonian cannot be solved exactly. It then presents the key equations of first order perturbation theory. The first order correction to the energy is given by the expectation value of the perturbation operator over the unperturbed ground state wavefunction. The first order correction to the wavefunction is expressed as a linear combination of unperturbed eigenstates.
Perturbation theory allows approximations of quantum systems where exact solutions cannot be easily determined. It involves splitting the Hamiltonian into known and perturbative terms. For the helium atom, the zero-order approximation treats it as two independent hydrogen atoms, yielding the wrong energy. The first-order approximation includes repulsion between electrons, giving a better but still incorrect energy. Variational theory provides an energy always greater than or equal to the actual energy.
Particle in a box- Application of Schrodinger wave equationRawat DA Greatt
The document summarizes key concepts from quantum chemistry, including:
1) It introduces the historical development of quantum mechanics from classical mechanics and discusses how quantum theory was needed to describe atomic and subatomic phenomena.
2) It then summarizes the particle-like and wave-like properties of light and matter and introduces the Schrodinger equation.
3) The document concludes by presenting the particle-in-a-box model and explaining how solving the Schrodinger equation for this system shows that a particle's energy is quantized into discrete energy levels when confined in a box.
this slide is introduce the postulates of quantum mechanics in which has all important definable objects is defined. so that presentation is helpful for the undergraduate students
Quantum mechanics is a branch of physics that deals with phenomena at microscopic scales, describing the wavelike and particle-like behavior of energy and matter. Erwin Schrödinger developed the wave equation and Schrödinger equation, which provide a mathematical description of quantum systems. Werner Heisenberg, Max Born, and Pascual Jordan created an equivalent formulation of quantum mechanics called matrix mechanics, which is the basis of Dirac's bra-ket notation for the wave function.
The document discusses the harmonic oscillator, which describes a physical system that oscillates around a central position at characteristic frequencies. The harmonic oscillator arises when a restoring force proportional to displacement opposes motion away from the central position, as seen with springs or vibrating strings. Key aspects discussed include the definition, history involving Planck and Einstein, the force-displacement relationship, derivation of the frequency equation, and potential energy function. Limitations of the harmonic oscillator model are that it predicts equal energy spacings and cannot describe bond breaking.
The Zeeman effect is the splitting of a spectral line into multiple spectral lines when in the presence of a magnetic field. It was first observed in 1896 by Dutch physicist Pieter Zeeman when he placed a sodium flame between magnetic poles and observed the broadening of spectral lines. Zeeman's discovery earned him the 1902 Nobel Prize in Physics. The pattern and amount of splitting provides information about the strength and presence of the magnetic field.
This document discusses the key principles of quantum physics including:
(1) The wave-particle duality of microparticles like electrons described by de Broglie's equation.
(2) Energy quantization described by Planck's equation.
(3) Heisenberg's uncertainty principle.
It describes how Schrodinger's equation is used to model the wave-like behavior of electrons in solids. The energy and behavior of electrons is quantized based on solutions to Schrodinger's equation under different boundary conditions, such as electrons confined in a potential well or interacting with a potential barrier. Quantum theory was needed to fully explain properties of electrons in solids and failures of classical free electron theory
This document discusses the simple harmonic oscillator. It defines a simple harmonic oscillator as an oscillator that is neither driven nor damped, with motion that is periodic and sinusoidal with constant amplitude. The acceleration of a body in simple harmonic motion is directly proportional to and directed towards the displacement from the equilibrium position. General equations for displacement, velocity, and acceleration as a function of time and other variables are provided. Quantum mechanical treatment of the simple harmonic oscillator is also summarized. Examples of simple harmonic oscillators include a mass on a spring and a simple pendulum in small angle approximation.
1. Nuclear models like the liquid drop model and shell model describe aspects of nuclear structure and behavior. The liquid drop model treats the nucleus like a liquid drop while the shell model treats nucleons as moving independently in nuclear orbits.
2. The shell model explains nuclear magic numbers and properties like spin and parity. Magic numbers correspond to nuclear stability when the number of protons or neutrons equals 2, 8, 20, 28, 50, 82, etc. The shell model accounts for magic numbers in terms of closed nuclear shells.
3. While insightful, nuclear models have limitations and do not fully describe all nuclear phenomena. The liquid drop model cannot explain magic numbers while the shell model fails to explain the stability of certain
This document discusses electron diffraction, including its principles and applications. Electron diffraction works by firing electrons at a sample and observing the scattering pattern, which can reveal information about the sample's structure. The key points covered are:
1. Electrons behave as waves and can diffract when passed through materials. Their wavelength depends on their energy.
2. Electron diffraction is used to determine bond lengths and angles in molecules by observing how the intensity of scattered electrons varies with angle.
3. Low-energy electron diffraction (LEED) analyzes surface structures by firing low-energy electrons at a sample's surface and observing the diffraction pattern.
4. LEED patterns reveal the two-dimensional arrangement of surface atoms
The document discusses the Schrodinger equation and methods to approximate solutions to it. It begins by defining the time-independent Schrodinger equation and its components. It then provides examples of writing out the Schrodinger equation for different chemical systems with varying numbers of electrons and nuclei. Approximation methods are needed because the Schrodinger equation can only be exactly solved for a few simple systems. Two approximation methods discussed are the variational method and perturbation theory. The variational method uses a trial wavefunction to variationally minimize the energy.
The document provides an overview of quantum mechanics concepts including:
- Erwin Schrodinger developed the Schrodinger wave equation which describes the energy and position of electrons.
- The time-dependent and time-independent Schrodinger equations are presented for 1D systems. Solutions include plane waves and wave packets.
- The postulates of quantum mechanics are outlined including the use of wavefunctions and Hermitian operators to represent physical quantities.
- Differences between the interpretations of quantum mechanics by Heisenberg and Schrodinger are briefly discussed.
This document introduces the Fermi-Dirac distribution function. It begins by discussing basic concepts like the Fermi level and Fermi energy. It then covers Fermi and Bose statistics, and the postulates of Fermi particles. The derivation of the Fermi-Dirac distribution function is shown, which gives the probability of a quantum state being occupied at a given energy and temperature. Graphs are presented showing how the distribution varies with different temperatures. The classical limit of the distribution is discussed. References are provided at the end.
1. Quantum mechanics began with Max Planck's paper in 1900 explaining black body radiation. It extends physics to small dimensions and includes classical laws as special cases.
2. Photoelectric effect shows that light behaves as particles called photons. Einstein's equation explained it using the photon energy.
3. Compton scattering showed that photons can collide with and transfer energy to electrons. The Compton wavelength was derived from this.
Nuclear Quadrupole Resonance Spectroscopy (NQR) is a chemical analysis technique that detects nuclear energy level transitions in the absence of a magnetic field through the absorption of radio frequency radiation. NQR is applicable to solids due to the quadrupole moment averaging to zero in liquids and gases. The interaction between a nucleus's quadrupole moment and the electric field gradient of its surroundings results in quantized energy levels. Transitions between these levels are detected as NQR spectra and provide information about electronic structure, hybridization, and charge distribution. NQR finds applications in studying charge transfer complexes, detecting crystal imperfections, and locating land mines.
Time Independent Perturbation Theory, 1st order correction, 2nd order correctionJames Salveo Olarve
The presentation is about how to solve the new energy levels and wave functions when the simple Hamiltonian is added by another term due to external effect (can be due to external field) .
The intended reader of this presentation were physics students. The author already assumed that the reader knows dirac braket notation.
This presentation shows a technique of how to solve for the approximate ground state energy using Schrodinger Equation in which the solution for wave function is not on hand
CHAPTER 6 Quantum Mechanics II
6.0 Partial differentials
6.1 The Schrödinger Wave Equation
6.2 Expectation Values
6.3 Infinite Square-Well Potential
6.4 Finite Square-Well Potential
6.5 Three-Dimensional Infinite-Potential Well
6.6 Simple Harmonic Oscillator
6.7 Barriers and Tunneling in some books an extra chapter due to its technical importance
The document discusses first order perturbation theory. It begins by introducing perturbation theory as an approximate method to solve the Schrodinger equation for complex quantum systems where the Hamiltonian cannot be solved exactly. It then presents the key equations of first order perturbation theory. The first order correction to the energy is given by the expectation value of the perturbation operator over the unperturbed ground state wavefunction. The first order correction to the wavefunction is expressed as a linear combination of unperturbed eigenstates.
Perturbation theory allows approximations of quantum systems where exact solutions cannot be easily determined. It involves splitting the Hamiltonian into known and perturbative terms. For the helium atom, the zero-order approximation treats it as two independent hydrogen atoms, yielding the wrong energy. The first-order approximation includes repulsion between electrons, giving a better but still incorrect energy. Variational theory provides an energy always greater than or equal to the actual energy.
Particle in a box- Application of Schrodinger wave equationRawat DA Greatt
The document summarizes key concepts from quantum chemistry, including:
1) It introduces the historical development of quantum mechanics from classical mechanics and discusses how quantum theory was needed to describe atomic and subatomic phenomena.
2) It then summarizes the particle-like and wave-like properties of light and matter and introduces the Schrodinger equation.
3) The document concludes by presenting the particle-in-a-box model and explaining how solving the Schrodinger equation for this system shows that a particle's energy is quantized into discrete energy levels when confined in a box.
this slide is introduce the postulates of quantum mechanics in which has all important definable objects is defined. so that presentation is helpful for the undergraduate students
Quantum mechanics is a branch of physics that deals with phenomena at microscopic scales, describing the wavelike and particle-like behavior of energy and matter. Erwin Schrödinger developed the wave equation and Schrödinger equation, which provide a mathematical description of quantum systems. Werner Heisenberg, Max Born, and Pascual Jordan created an equivalent formulation of quantum mechanics called matrix mechanics, which is the basis of Dirac's bra-ket notation for the wave function.
The document discusses the harmonic oscillator, which describes a physical system that oscillates around a central position at characteristic frequencies. The harmonic oscillator arises when a restoring force proportional to displacement opposes motion away from the central position, as seen with springs or vibrating strings. Key aspects discussed include the definition, history involving Planck and Einstein, the force-displacement relationship, derivation of the frequency equation, and potential energy function. Limitations of the harmonic oscillator model are that it predicts equal energy spacings and cannot describe bond breaking.
The Zeeman effect is the splitting of a spectral line into multiple spectral lines when in the presence of a magnetic field. It was first observed in 1896 by Dutch physicist Pieter Zeeman when he placed a sodium flame between magnetic poles and observed the broadening of spectral lines. Zeeman's discovery earned him the 1902 Nobel Prize in Physics. The pattern and amount of splitting provides information about the strength and presence of the magnetic field.
This document discusses the key principles of quantum physics including:
(1) The wave-particle duality of microparticles like electrons described by de Broglie's equation.
(2) Energy quantization described by Planck's equation.
(3) Heisenberg's uncertainty principle.
It describes how Schrodinger's equation is used to model the wave-like behavior of electrons in solids. The energy and behavior of electrons is quantized based on solutions to Schrodinger's equation under different boundary conditions, such as electrons confined in a potential well or interacting with a potential barrier. Quantum theory was needed to fully explain properties of electrons in solids and failures of classical free electron theory
This document discusses the simple harmonic oscillator. It defines a simple harmonic oscillator as an oscillator that is neither driven nor damped, with motion that is periodic and sinusoidal with constant amplitude. The acceleration of a body in simple harmonic motion is directly proportional to and directed towards the displacement from the equilibrium position. General equations for displacement, velocity, and acceleration as a function of time and other variables are provided. Quantum mechanical treatment of the simple harmonic oscillator is also summarized. Examples of simple harmonic oscillators include a mass on a spring and a simple pendulum in small angle approximation.
1. Nuclear models like the liquid drop model and shell model describe aspects of nuclear structure and behavior. The liquid drop model treats the nucleus like a liquid drop while the shell model treats nucleons as moving independently in nuclear orbits.
2. The shell model explains nuclear magic numbers and properties like spin and parity. Magic numbers correspond to nuclear stability when the number of protons or neutrons equals 2, 8, 20, 28, 50, 82, etc. The shell model accounts for magic numbers in terms of closed nuclear shells.
3. While insightful, nuclear models have limitations and do not fully describe all nuclear phenomena. The liquid drop model cannot explain magic numbers while the shell model fails to explain the stability of certain
This document discusses electron diffraction, including its principles and applications. Electron diffraction works by firing electrons at a sample and observing the scattering pattern, which can reveal information about the sample's structure. The key points covered are:
1. Electrons behave as waves and can diffract when passed through materials. Their wavelength depends on their energy.
2. Electron diffraction is used to determine bond lengths and angles in molecules by observing how the intensity of scattered electrons varies with angle.
3. Low-energy electron diffraction (LEED) analyzes surface structures by firing low-energy electrons at a sample's surface and observing the diffraction pattern.
4. LEED patterns reveal the two-dimensional arrangement of surface atoms
The document discusses the Schrodinger equation and methods to approximate solutions to it. It begins by defining the time-independent Schrodinger equation and its components. It then provides examples of writing out the Schrodinger equation for different chemical systems with varying numbers of electrons and nuclei. Approximation methods are needed because the Schrodinger equation can only be exactly solved for a few simple systems. Two approximation methods discussed are the variational method and perturbation theory. The variational method uses a trial wavefunction to variationally minimize the energy.
The document provides an overview of quantum mechanics concepts including:
- Erwin Schrodinger developed the Schrodinger wave equation which describes the energy and position of electrons.
- The time-dependent and time-independent Schrodinger equations are presented for 1D systems. Solutions include plane waves and wave packets.
- The postulates of quantum mechanics are outlined including the use of wavefunctions and Hermitian operators to represent physical quantities.
- Differences between the interpretations of quantum mechanics by Heisenberg and Schrodinger are briefly discussed.
The document provides an outline for a course on quantum mechanics. It discusses key topics like the time-dependent Schrodinger equation, eigenvalues and eigenfunctions, boundary conditions for wave functions, and applications like the particle in a box model. Specific solutions to the Schrodinger equation are explored for stationary states with definite energy, including the wave function for a free particle and the quantization of energy for a particle confined to a one-dimensional box.
The document discusses the Compton effect, which describes the scattering of high frequency electromagnetic radiation (x-rays or gamma rays) when interacting with matter. When radiation scatters off of electrons in an atom, the radiation wavelength increases. This is because some of the radiation's energy is transferred to the electron. The Compton effect can be explained using conservation of energy and momentum. It demonstrated that the difference between the scattered and incident wavelengths is directly proportional to the energy and momentum transfers during collision.
The document discusses the Schrödinger equation, which describes the wave-like behavior of matter and microscopic particles. It introduces the time-dependent and time-independent Schrödinger equations. The time-independent Schrödinger equation can be derived by separating the time and space dependencies of the wave function for situations where the potential is independent of time. Solving the time-independent Schrödinger equation provides the possible energy states of the system.
This document summarizes classical dynamics and small amplitude oscillations. It discusses oscillatory motion near equilibrium positions and developing the theory using Lagrange's equations. Normal modes of coupled oscillating systems are explored, where the normal coordinates represent eigenvectors that oscillate at characteristic frequencies. The principles of superposition and matrix representations are used to analyze examples like two coupled pendulums and a system of two masses connected by three springs.
The WKB approximation is a method to find approximate solutions to the Schrodinger equation. It was developed in 1926 by Wentzel, Kramer, and Brillouin. The approximation assumes the wavefunction is an exponentially varying function with amplitude and phase that change slowly compared to the de Broglie wavelength. It can be used to obtain approximate solutions and energy eigenvalues for systems where the classical limit is valid. The approximation breaks down near classical turning points where the particle's energy is equal to the potential energy. The document provides examples of using the WKB approximation to solve the time-independent Schrodinger equation in one dimension for cases where the particle's energy is both greater than and less than the potential energy.
The document discusses the classical and quantum mechanical treatment of the simple harmonic oscillator.
Classically, the simple harmonic oscillator exhibits sinusoidal motion with a single resonant frequency, where the restoring force is proportional to displacement from equilibrium. Quantum mechanically, the energy levels of the 1D harmonic oscillator are quantized and equally spaced. The wave functions are solutions of the Schrodinger equation and can be written as products of Hermite polynomials and Gaussian functions. The energy eigenstates of the 1D harmonic oscillator are (n+1/2)ħω, where n is the vibrational quantum number.
The document discusses Newton's applications and special theory of relativity. It covers topics like periodic motion, oscillation, restoring force, damping force, simple harmonic oscillations, examples of SHO like simple pendulum and loaded vertical spring. It also discusses damped harmonic oscillations including underdamped, overdamped and critically damped cases. Small oscillations in a bound system and molecular vibrations are also summarized.
In tis slide, an introduction to string theory has been given. Apart from that, a simple proof of 26 dimensions of bosonic string theory is given (following Zwiebach's approach).
I explained this presentation in two parts (on my YouTube channel). Here are the links
_______________________________________________
Part 1
https://www.youtube.com/watch?v=QQA4JQ6Y-eo&list=PLDpqC3uXLZGl0cDod6g30PcjeJ4DAZWhp
_______________________________________________
Part 2
https://www.youtube.com/watch?v=vhLCtLn79jE&list=PLDpqC3uXLZGl0cDod6g30PcjeJ4DAZWhp&index=2
_______________________________________________
This document provides an overview of quantum mechanics concepts including the Schrödinger wave equation, expectation values, infinite and finite square well potentials, the three-dimensional infinite potential well, the simple harmonic oscillator, barriers and tunneling. Key topics covered include the quantization of energy, boundary conditions, normalization, penetration depth, degeneracy, reflection and transmission probabilities, and an explanation of tunneling using the uncertainty principle. Real world examples of these concepts like alpha particle decay are also discussed.
This document provides an overview of quantum mechanics topics including:
1) The Schrödinger wave equation and its time-dependent and time-independent forms.
2) Expectation values and how they are used to calculate probabilities, momentum, position, and energy.
3) Specific quantum systems like infinite and finite square wells and simple harmonic oscillators. It also discusses quantization, degeneracy, and other concepts.
4) Barrier penetration and tunneling, where particles can pass through barriers that would be forbidden classically.
The document covers many fundamental aspects of quantum mechanics through examining various quantum systems and potentials.
Lecture Notes: EEEC6430310 Electromagnetic Fields And Waves - Maxwell's Equa...AIMST University
1) The document discusses Maxwell's equations for electromagnetic fields and waves, including Faraday's law, Ampere's law, and Gauss' laws.
2) It covers Pointing's theorem, which relates electromagnetic energy density and power flow. Power flow is represented by the Poynting vector.
3) The document examines plane electromagnetic waves in different media, deriving the wave equation and showing that waves propagate at the speed of light.
This course covers gas dynamics, including basic equations of motion, mass conservation, fundamental processes like steady flows and shocks, and applications like stellar winds and supernova remnants. It introduces key concepts like the equation of motion for fluids, pressure forces, and flow fields. The lectures will define important terms like mass density, velocity, and acceleration of fluid elements. Equations like the Navier-Stokes equations will be examined, relating fluid acceleration to forces like pressure and viscosity.
The Harmonic Oscillator/ Why do we need to study harmonic oscillator model?.pptxtsdalmutairi
The harmonic oscillator system is important as a model for molecular vibrations. The vibrational energy levels of a diatomic molecule can be approximated by the levels of a harmonic oscillator
At first, we are going to study harmonic oscillator from a classical mechanical perspective and then will discuss the allowed energy levels and the corresponding wave function of the harmonic oscillator from a quantum mechanical point of view.
Later on we are going to describe the infrared spectrum of a diatomic molecules using the quantum mechanical energies. Also we are going to figure out how to determine molecular force constant.
Finally, we are going to learn selection rules for a harmonic oscillator and the normal coordinates which describe the vibrational motion of polyatomic molecules.
The document summarizes the quantum mechanical treatment of the harmonic oscillator. It begins by reviewing classical harmonic motion and the classical harmonic oscillator equation. It then introduces the quantum mechanical treatment using the Schrodinger equation. Dimensionless units of energy and length are defined in terms of the oscillator frequency and mass. The energies and wavefunctions of the harmonic oscillator are then derived and illustrated. Specific examples are given for the HCl, HBr, and HI diatomic molecules.
Unit 1 Quantum Mechanics_230924_162445.pdfSwapnil947063
1) Quantum mechanics is needed to explain phenomena at the microscopic level that classical physics cannot, such as the stability of atoms and line spectra of hydrogen.
2) According to de Broglie's hypothesis, all matter exhibits wave-particle duality - particles are associated with waves called matter waves. The wavelength of these matter waves is given by de Broglie's equation.
3) In quantum mechanics, the wave function ψ describes the wave properties of a particle. The probability of finding a particle in a region is given by the absolute square of the wave function |ψ|2 in that region.
Gravitational field and potential, escape velocity, universal gravitational l...lovizabasharat
What is Escape Velocity-its derivation-examples-applications
Universal Gravitational Law-Derivation and Examples
Gravitational Field And Gravitational Potential-Derivation, Realation and numericals
Radial Velocity and acceleration-derivation and examples
Transverse Velocity and acceleration and examples
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.
Travis Hills' Endeavors in Minnesota: Fostering Environmental and Economic Pr...Travis Hills MN
Travis Hills of Minnesota developed a method to convert waste into high-value dry fertilizer, significantly enriching soil quality. By providing farmers with a valuable resource derived from waste, Travis Hills helps enhance farm profitability while promoting environmental stewardship. Travis Hills' sustainable practices lead to cost savings and increased revenue for farmers by improving resource efficiency and reducing waste.
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.
EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Weste...Sérgio Sacani
Context. With a mass exceeding several 104 M⊙ and a rich and dense population of massive stars, supermassive young star clusters
represent the most massive star-forming environment that is dominated by the feedback from massive stars and gravitational interactions
among stars.
Aims. In this paper we present the Extended Westerlund 1 and 2 Open Clusters Survey (EWOCS) project, which aims to investigate
the influence of the starburst environment on the formation of stars and planets, and on the evolution of both low and high mass stars.
The primary targets of this project are Westerlund 1 and 2, the closest supermassive star clusters to the Sun.
Methods. The project is based primarily on recent observations conducted with the Chandra and JWST observatories. Specifically,
the Chandra survey of Westerlund 1 consists of 36 new ACIS-I observations, nearly co-pointed, for a total exposure time of 1 Msec.
Additionally, we included 8 archival Chandra/ACIS-S observations. This paper presents the resulting catalog of X-ray sources within
and around Westerlund 1. Sources were detected by combining various existing methods, and photon extraction and source validation
were carried out using the ACIS-Extract software.
Results. The EWOCS X-ray catalog comprises 5963 validated sources out of the 9420 initially provided to ACIS-Extract, reaching a
photon flux threshold of approximately 2 × 10−8 photons cm−2
s
−1
. The X-ray sources exhibit a highly concentrated spatial distribution,
with 1075 sources located within the central 1 arcmin. We have successfully detected X-ray emissions from 126 out of the 166 known
massive stars of the cluster, and we have collected over 71 000 photons from the magnetar CXO J164710.20-455217.
hematic appreciation test is a psychological assessment tool used to measure an individual's appreciation and understanding of specific themes or topics. This test helps to evaluate an individual's ability to connect different ideas and concepts within a given theme, as well as their overall comprehension and interpretation skills. The results of the test can provide valuable insights into an individual's cognitive abilities, creativity, and critical thinking skills
The ability to recreate computational results with minimal effort and actionable metrics provides a solid foundation for scientific research and software development. When people can replicate an analysis at the touch of a button using open-source software, open data, and methods to assess and compare proposals, it significantly eases verification of results, engagement with a diverse range of contributors, and progress. However, we have yet to fully achieve this; there are still many sociotechnical frictions.
Inspired by David Donoho's vision, this talk aims to revisit the three crucial pillars of frictionless reproducibility (data sharing, code sharing, and competitive challenges) with the perspective of deep software variability.
Our observation is that multiple layers — hardware, operating systems, third-party libraries, software versions, input data, compile-time options, and parameters — are subject to variability that exacerbates frictions but is also essential for achieving robust, generalizable results and fostering innovation. I will first review the literature, providing evidence of how the complex variability interactions across these layers affect qualitative and quantitative software properties, thereby complicating the reproduction and replication of scientific studies in various fields.
I will then present some software engineering and AI techniques that can support the strategic exploration of variability spaces. These include the use of abstractions and models (e.g., feature models), sampling strategies (e.g., uniform, random), cost-effective measurements (e.g., incremental build of software configurations), and dimensionality reduction methods (e.g., transfer learning, feature selection, software debloating).
I will finally argue that deep variability is both the problem and solution of frictionless reproducibility, calling the software science community to develop new methods and tools to manage variability and foster reproducibility in software systems.
Exposé invité Journées Nationales du GDR GPL 2024
Remote Sensing and Computational, Evolutionary, Supercomputing, and Intellige...University of Maribor
Slides from talk:
Aleš Zamuda: Remote Sensing and Computational, Evolutionary, Supercomputing, and Intelligent Systems.
11th International Conference on Electrical, Electronics and Computer Engineering (IcETRAN), Niš, 3-6 June 2024
Inter-Society Networking Panel GRSS/MTT-S/CIS Panel Session: Promoting Connection and Cooperation
https://www.etran.rs/2024/en/home-english/
ESPP presentation to EU Waste Water Network, 4th June 2024 “EU policies driving nutrient removal and recycling
and the revised UWWTD (Urban Waste Water Treatment Directive)”
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.
Current Ms word generated power point presentation covers major details about the micronuclei test. It's significance and assays to conduct it. It is used to detect the micronuclei formation inside the cells of nearly every multicellular organism. It's formation takes place during chromosomal sepration at metaphase.
2. SCHRÖDINGER’S WAVE EQUATION
Schrödinger’s Time Dependent
Equation
In most situations, potential
energy is a function of position as
well as time.
(-
ℏ𝟐
𝟐𝒎
𝛁𝟐 + 𝑽)𝜳(𝒙, 𝒚, 𝒛, 𝒕) = 𝒊ℏ
𝜕𝛹
𝜕𝑡
Schrödinger’s Time Independent
Equation
In several situations, potential energy
is a function of position alone and
doesn’t depend upon time.
Schrödinger’s time independent
equation is also known as the steady
state equation.
(-
ℏ𝟐
𝟐𝒎
𝛁𝟐
+ 𝑽)𝜳(𝒙, 𝒚, 𝒛) = 𝑬𝜳(𝒙, 𝒚, 𝒛)
Schrödinger’s equation is a wave equation in terms of the variable 𝛹 and
represents the fundamental equation in quantum mechanics.
3. DERIVATION
Consider a system of stationary waves associated with a particle
moving with velocity, ‘v’ and 𝛹 = 𝛹 (x, y, z, t) be the wave function.
The differential equation of the 3-D wave motion is given as:
𝜕2
𝛹
𝜕𝑡2
= 𝑣2
𝜕2
𝛹
𝜕𝑥2
+
𝜕2
𝛹
𝜕𝑦
2 +
𝜕2
𝛹
𝜕𝑧2
= 𝑣2∇2𝛹
The solution of the above equation is of the form:
𝛹 = 𝛹0 sin 𝜔𝑡 = 𝛹0 sin 2𝜋𝜃𝑡
⇒
𝜕𝛹
𝜕𝑡
= 𝛹0 2𝜋𝜃 cos 2𝜋𝜃𝑡
7. 1. Particle in a box/ Infinite potential well:
Using Schrödinger’s Time Independent
Equation, we get the following wavefunction and eigen
values for this case,
𝛹n(x)=
2
𝑎
sin
𝑛𝜋𝑥
𝑎
where n = 1,2,3,…
𝐸𝑛 =
𝑛2𝜋2ℏ2
2𝑚𝑎2
8. 2. Quantum Harmonic Oscillator:
Using Schrödinger’s Time Independent
Equation, we get the following wavefunction and eigen values for
this case,
𝐸𝑛 = 𝑛 +
1
2
ℏ𝜔
9. 3. Quantum Mechanical Tunnelling Effect:
• Quantum mechanically, if E > 𝑉0 , then there is
always some probability of reflection at x = 0 and
at x = a.
• Also, if E < 𝑉0 , then there is always some
probability of penetration into the barrier.
• In this case we apply Schrödinger’s Time
Independent
• Equation to understand quantum mechanical
tunnelling effect.
V 𝒙 =
𝑽𝟎 𝟎 < 𝐱 < 𝐚
∞ 𝐞𝐥𝐬𝐞𝐰𝐡𝐞𝐫𝐞
10. MCQ 1: Which of these is the mathematical
representation of Hamiltonian operator?
1) -
ℏ𝟐
𝟐𝒎
∇ + 𝑽
2) -
ℏ𝟐
𝟐𝒎
𝛁𝟐
+ 𝑽
3) -
ℏ𝟐
𝟒𝒎
𝛁𝟐
+ 𝑽
4) -
ℏ𝟐
𝟒𝒎
∇ +𝑽
11. MCQ 2: Which of the following option is
true?
Statement 1: Schrödinger’s time independent equation is also known as the steady
state equation.
Statement 2: Schrödinger’s time dependent equation is also known as the steady
state equation.
1) Both the statements are true.
2) Only Statement 2 is true.
3) None of them is true.
4) Only Statement 1 is true.