9.02 Quantum Mechanics and the Schrodinger Equation

Total Page:16

File Type:pdf, Size:1020Kb

9.02 Quantum Mechanics and the Schrodinger Equation 9.02 Quantum Mechanics and The Schrodinger Equation Dr. Fred Omega Garces Chemistry 152 Miramar College 1 9.2 Quantum Mechanics and The Schrodinger Equation 05.2015 Wave Treatment of the Atom What is the Schrodinger Wave Equation? How does the solution of the Schrodinger Wave equation lead to a model of the atom ? Representation of Orbitals Quantum Numbers / Restrictions n - Energy; Principal Quantum #, Shell, n=1,2,3 ... l - orbital shape; Azimuthal Quantum #, l = 0,1,2,3 ...n-1 ml - orbital orientation, Magnetic Quantum #, m l = - l ...0...+ l ms - electron spin, Direction of electron spin, ms = +1/2, -1/2 Arrangement of electrons Pictorial - illustration of shells in an atom Energy Diagram- Energy level depicting the relative energies Mnemonic - Upside down “Hotel del Orbital” Orbital Block Diagram- electron box illustrating e- config. e- Configuration - Nomenclature of e- configuration. Electron configuration Notation of the electron address 2 9.2 Quantum Mechanics and The Schrodinger Equation 05.2015 Schrodinger Wave Equation Properties of the Schrodinger equation provides information about the electronic arrangement of each atom. H Ψ = EΨ H-Hamiltonian Operator E-Eigen Value (Math function) Total energy of the atom i.e. ex, ln, yx, !, E Sum of P.E.; attraction of p+, e- and K.E. of moving e-. Ψ -Psi - wave function: wave properties Ψ2 -probability distribution 3 9.2 Quantum Mechanics and The Schrodinger Equation 05.2015 Significance of the Schrodinger Equation Properties of the Schrodinger is mathematically sophisticated, but it has four important features that can be appreciated without understanding how to solve the equation. 1. H - Hamiltonian is different for every atom, ion or molecule. 2. Ψ - Wave function has wave properties and has spatial variables: Ψ = ψ(x,y,z) • Ψ - is the math function that gives information of the electron at any point in space; shell and orbital. • Ψ2 - is the probability of finding e- at any point in space (Probability distribution). 3. Schrodinger equation has solution only for specific value of Energy. This is the quantum condition. 4. Schrodinger equation has solution for any atom or molecule and has an infinite number of solution. Molecules or atoms have infinite number of discrete energies En and each of these correspond to a different Ψn 4 9.2 Quantum Mechanics and The Schrodinger Equation 05.2015 Electron Address and Ψ When e- is promoted to new orbital there is a new: Ψ - wave function for e - at ground state. Ψ2 - probability of e- distribution about atom E - Energy of electron e e Ψ - wave function for e - at ground state. Ψ2 - probability of e- distribution about atom E - energy of electron Many Wavefunction Ψ are acceptable with each Ψ having unique set of quantum numbers. Quantum number - Address of each electron; yields size, shape, orientation and spin of e- It is essential to realize that an atomic orbital bears no resemblance whatsoever to an “orbital” in the Bohr model: the orbital is a mathematical function with no independent physical reality. 5 9.2 Quantum Mechanics and The Schrodinger Equation 05.2015 Representation of Orbitals Classic Orbit: Orbital (3D) Probability distribution 3s 1s 6 9.2 Quantum Mechanics and The Schrodinger Equation 05.2015 Ψ, Ψ2 and Atomic shells Ψ - Schrodinger equation. Electron density plots, Math formula electron cloud depictions, - describing e and radial probability with particle- distribution plots for three wave duality s orbitals. Information for character. each of the s orbital is shown as a plot of electron density (top), a cloud representation of the electron density (middle), in Orbital which shading coincides with density peaks in the plot above, and picture a radial probability distribution (bottom) that shows where the electrons Ψ2 - Probability of spends its time e- distribution from center of nucleus 7 9.2 Quantum Mechanics and The Schrodinger Equation 05.2015 Quantum numbers 4 Parameters (quantum number) which provide address of each electron of an atom. Quantum numbers give probability of electron location in 3-dimensional space. Description Quantum Name Value Energy n-Shell Principal Quantum# n = 1,2,3,...∞ shell - Probability Vol - info. of e location from nucleus. Orbital l - subshell Azimuthal Quantum # l =0,1,2,3,...n-1 Shape Angular momentum l =0, s-suborbital info. of shape of orbital l =1, p-suborbital Orbital ml Magnetic Quantum # ml = - l , - l +1,.. 0, ... l +1, l Orientation info. on the orbital Total = 2 l +1 state orientation Electron ms Electron spin Quantum # ms = +1/2 or -1/2 spin info. on direction of - e spin. 8 9.2 Quantum Mechanics and The Schrodinger Equation 05.2015 Relationship of Quantum Numbers Quantum numbers are dependent on each other Shell Subshell Orbital l = 3 d +2 +1 0 -1 -2 n = 3 l = 1 p +1 0 -1 l = 0 s 0 l = 1 p +1 0 -1 n = 2 l = 0 s 0 n = 1 l = 0 s 0 n l ml 9 9.2 Quantum Mechanics and The Schrodinger Equation 05.2015 Quantum Numbers and electron Address Your address is defined by Your name Your street Similarly, in an atom each Your City electron has a unique . Your State The shell (Energy level-Size) Zip Code n- Principal Quantum Number. The Orbital Orientation (Shape) l -azimuthal Quantum number. The suborbital probability Volume Address Code: ml - suborbital orientation n = 1, 2, 3, ... (Orientation) ∞ Spin of electron l = 0, 1, 2, ... n-1 → s, p, d,... ms- Magnetic Spin ml = -l... 0 ... l → (p) px, py, pz → (d) dxy, dyz, dxz, dx2-y2 , dx2 ms → +1/2, -1/2 10 9.2 Quantum Mechanics and The Schrodinger Equation 05.2015 Wavefunction Ψ and Quantum number (n) n Principle Quantum Number Size of shell which determines the energy. n = 1,2,3,4,... n =4 n =3 n =2 n =1 11 9.2 Quantum Mechanics and The Schrodinger Equation 05.2015 Wavefunction Ψ and Quantum number (l ) l Azimuthal Quantum Number (Angular momentum) Determines the Shape of the orbital. l = 0, 1, 2, ... n-1 l = 0 l = 1 l =2 l = 3 ... s p d f 12 9.2 Quantum Mechanics and The Schrodinger Equation 05.2015 Wavefunction Ψ and Quantum number ( ml ) ml Magnetic Quantum Number Orientation of Orbital (Sub Orbital) ml = 0, 1, 2, ... n-1 l = 0 l = 1 l =2 l = 3 ... m = 0 m = -1 ,0 ,1, m =2, -1 ,0 ,1, 2 m = -3, -2, -1, 0, 1, 2, 3 l l l l s p d f Lobes and nodes? 13 9.2 Quantum Mechanics and The Schrodinger Equation 05.2015 Wavefunction Ψ and Quantum number ( ms ) ms Electron Spin Quantum Number Spin orientation of electron. ms = - 1/2 , +1/2 14 9.2 Quantum Mechanics and The Schrodinger Equation 05.2015 Atomic Orbitals Shown below are orbitals density plots and Ψ2 vs. r plots for the 1s, 2s, 2p and 3p orbitals 1s 2s 2p 3p 15 9.2 Quantum Mechanics and The Schrodinger Equation 05.2015 Ψ2 and Atomic Orbitals Electron density plots for specific orbitals Electron density plots Ψ2 for 1s, 2s and 3s orbitals for the 1s, 2s, and 3s atomic orbitals of the 1s hydrogen atom. The vertical lines indicate 2s the value of r where the 90% contour surface would be located. 3s Notice that this value is about four times as large for 2s as for 1s 2 Ψ and about nine times as large for 3s as far 1s. r distance from the nucleus 16 9.2 Quantum Mechanics and The Schrodinger Equation 05.2015 Ψ2 and Atomic Orbitals Electron density plots for 1s, 2s, 2p, 3s, 3p, and 3d orbitals for the hydrogen atom. All orbitals belonging to the same principle quantum number, n has their maximum electron density occurring at about the same distance from the nucleus. In other words, all orbitals with the same principle 3d quantum number are about the same size. 2p 3p 1s 2s 3s 3s 3p 3d 1s 2s 2p 17 9.2 Quantum Mechanics and The Schrodinger Equation 05.2015 Shells and Orbitals and Atomic Structure f d s p Shells of an atom contain a number of stacked orbitals 4 3 2 1 18 9.2 Quantum Mechanics and The Schrodinger Equation 05.2015 Relative Energies for Shells and Orbitals p ∞ s d f 8 Not only do shells 7 have different 6 energies (n levels), 5 but different suborbitals have 4 different energies Note that the d and f-orbitals have 3 energies which overlap energy level of the s-orbital. 2 Relative Energies of the 1 orbitals 19 9.2 Quantum Mechanics and The Schrodinger Equation 05.2015 Summary The electron’s wave function (ϕ, atomic orbital) is a mathematical description of the electron's wavelike motion in an atom. Each wave function is associated with one of the atom’s allowed energy states. The probability of finding the electron at a particular location is represented by ϕ2. An electron density diagram and a radial probability distribution plot show how the electron occupies the space near the nucleus for a particular energy level. Three features of the atomic orbital are described by quantum numbers: size (n), shape (l), and orientation (ml). Orbitals are part of sublevels (defined by n and l), which are part of an energy level (defined by n). A sublevel with l =0 has a spherical (s) orbital (no nodes); one with l =1 has two-lobed (p) orbitals (one node); and one with l =2 has four lobed (d) orbitals (two nodes). For the H atom, the energy levels depend only on the n value.
Recommended publications
  • Unit 1 Old Quantum Theory
    UNIT 1 OLD QUANTUM THEORY Structure Introduction Objectives li;,:overy of Sub-atomic Particles Earlier Atom Models Light as clectromagnetic Wave Failures of Classical Physics Black Body Radiation '1 Heat Capacity Variation Photoelectric Effect Atomic Spectra Planck's Quantum Theory, Black Body ~diation. and Heat Capacity Variation Einstein's Theory of Photoelectric Effect Bohr Atom Model Calculation of Radius of Orbits Energy of an Electron in an Orbit Atomic Spectra and Bohr's Theory Critical Analysis of Bohr's Theory Refinements in the Atomic Spectra The61-y Summary Terminal Questions Answers 1.1 INTRODUCTION The ideas of classical mechanics developed by Galileo, Kepler and Newton, when applied to atomic and molecular systems were found to be inadequate. Need was felt for a theory to describe, correlate and predict the behaviour of the sub-atomic particles. The quantum theory, proposed by Max Planck and applied by Einstein and Bohr to explain different aspects of behaviour of matter, is an important milestone in the formulation of the modern concept of atom. In this unit, we will study how black body radiation, heat capacity variation, photoelectric effect and atomic spectra of hydrogen can be explained on the basis of theories proposed by Max Planck, Einstein and Bohr. They based their theories on the postulate that all interactions between matter and radiation occur in terms of definite packets of energy, known as quanta. Their ideas, when extended further, led to the evolution of wave mechanics, which shows the dual nature of matter
    [Show full text]
  • Quantum Theory of the Hydrogen Atom
    Quantum Theory of the Hydrogen Atom Chemistry 35 Fall 2000 Balmer and the Hydrogen Spectrum n 1885: Johann Balmer, a Swiss schoolteacher, empirically deduced a formula which predicted the wavelengths of emission for Hydrogen: l (in Å) = 3645.6 x n2 for n = 3, 4, 5, 6 n2 -4 •Predicts the wavelengths of the 4 visible emission lines from Hydrogen (which are called the Balmer Series) •Implies that there is some underlying order in the atom that results in this deceptively simple equation. 2 1 The Bohr Atom n 1913: Niels Bohr uses quantum theory to explain the origin of the line spectrum of hydrogen 1. The electron in a hydrogen atom can exist only in discrete orbits 2. The orbits are circular paths about the nucleus at varying radii 3. Each orbit corresponds to a particular energy 4. Orbit energies increase with increasing radii 5. The lowest energy orbit is called the ground state 6. After absorbing energy, the e- jumps to a higher energy orbit (an excited state) 7. When the e- drops down to a lower energy orbit, the energy lost can be given off as a quantum of light 8. The energy of the photon emitted is equal to the difference in energies of the two orbits involved 3 Mohr Bohr n Mathematically, Bohr equated the two forces acting on the orbiting electron: coulombic attraction = centrifugal accelleration 2 2 2 -(Z/4peo)(e /r ) = m(v /r) n Rearranging and making the wild assumption: mvr = n(h/2p) n e- angular momentum can only have certain quantified values in whole multiples of h/2p 4 2 Hydrogen Energy Levels n Based on this model, Bohr arrived at a simple equation to calculate the electron energy levels in hydrogen: 2 En = -RH(1/n ) for n = 1, 2, 3, 4, .
    [Show full text]
  • Principal, Azimuthal and Magnetic Quantum Numbers and the Magnitude of Their Values
    268 A Textbook of Physical Chemistry – Volume I Principal, Azimuthal and Magnetic Quantum Numbers and the Magnitude of Their Values The Schrodinger wave equation for hydrogen and hydrogen-like species in the polar coordinates can be written as: 1 휕 휕휓 1 휕 휕휓 1 휕2휓 8휋2휇 푍푒2 (406) [ (푟2 ) + (푆푖푛휃 ) + ] + (퐸 + ) 휓 = 0 푟2 휕푟 휕푟 푆푖푛휃 휕휃 휕휃 푆푖푛2휃 휕휙2 ℎ2 푟 After separating the variables present in the equation given above, the solution of the differential equation was found to be 휓푛,푙,푚(푟, 휃, 휙) = 푅푛,푙. 훩푙,푚. 훷푚 (407) 2푍푟 푘 (408) 3 푙 푘=푛−푙−1 (−1)푘+1[(푛 + 푙)!]2 ( ) 2푍 (푛 − 푙 − 1)! 푍푟 2푍푟 푛푎 √ 0 = ( ) [ 3] . exp (− ) . ( ) . ∑ 푛푎0 2푛{(푛 + 푙)!} 푛푎0 푛푎0 (푛 − 푙 − 1 − 푘)! (2푙 + 1 + 푘)! 푘! 푘=0 (2푙 + 1)(푙 − 푚)! 1 × √ . 푃푚(퐶표푠 휃) × √ 푒푖푚휙 2(푙 + 푚)! 푙 2휋 It is obvious that the solution of equation (406) contains three discrete (n, l, m) and three continuous (r, θ, ϕ) variables. In order to be a well-behaved function, there are some conditions over the values of discrete variables that must be followed i.e. boundary conditions. Therefore, we can conclude that principal (n), azimuthal (l) and magnetic (m) quantum numbers are obtained as a solution of the Schrodinger wave equation for hydrogen atom; and these quantum numbers are used to define various quantum mechanical states. In this section, we will discuss the properties and significance of all these three quantum numbers one by one. Principal Quantum Number The principal quantum number is denoted by the symbol n; and can have value 1, 2, 3, 4, 5…..∞.
    [Show full text]
  • Vibrational Quantum Number
    Fundamentals in Biophotonics Quantum nature of atoms, molecules – matter Aleksandra Radenovic [email protected] EPFL – Ecole Polytechnique Federale de Lausanne Bioengineering Institute IBI 26. 03. 2018. Quantum numbers •The four quantum numbers-are discrete sets of integers or half- integers. –n: Principal quantum number-The first describes the electron shell, or energy level, of an atom –ℓ : Orbital angular momentum quantum number-as the angular quantum number or orbital quantum number) describes the subshell, and gives the magnitude of the orbital angular momentum through the relation Ll2 ( 1) –mℓ:Magnetic (azimuthal) quantum number (refers, to the direction of the angular momentum vector. The magnetic quantum number m does not affect the electron's energy, but it does affect the probability cloud)- magnetic quantum number determines the energy shift of an atomic orbital due to an external magnetic field-Zeeman effect -s spin- intrinsic angular momentum Spin "up" and "down" allows two electrons for each set of spatial quantum numbers. The restrictions for the quantum numbers: – n = 1, 2, 3, 4, . – ℓ = 0, 1, 2, 3, . , n − 1 – mℓ = − ℓ, − ℓ + 1, . , 0, 1, . , ℓ − 1, ℓ – –Equivalently: n > 0 The energy levels are: ℓ < n |m | ≤ ℓ ℓ E E 0 n n2 Stern-Gerlach experiment If the particles were classical spinning objects, one would expect the distribution of their spin angular momentum vectors to be random and continuous. Each particle would be deflected by a different amount, producing some density distribution on the detector screen. Instead, the particles passing through the Stern–Gerlach apparatus are deflected either up or down by a specific amount.
    [Show full text]
  • Lecture 3: Particle in a 1D Box
    Lecture 3: Particle in a 1D Box First we will consider a free particle moving in 1D so V (x) = 0. The TDSE now reads ~2 d2ψ(x) = Eψ(x) −2m dx2 which is solved by the function ψ = Aeikx where √2mE k = ± ~ A general solution of this equation is ψ(x) = Aeikx + Be−ikx where A and B are arbitrary constants. It can also be written in terms of sines and cosines as ψ(x) = C sin(kx) + D cos(kx) The constants appearing in the solution are determined by the boundary conditions. For a free particle that can be anywhere, there is no boundary conditions, so k and thus E = ~2k2/2m can take any values. The solution of the form eikx corresponds to a wave travelling in the +x direction and similarly e−ikx corresponds to a wave travelling in the -x direction. These are eigenfunctions of the momentum operator. Since the particle is free, it is equally likely to be anywhere so ψ∗(x)ψ(x) is independent of x. Incidently, it cannot be normalized because the particle can be found anywhere with equal probability. 1 Now, let us confine the particle to a region between x = 0 and x = L. To do this, we choose our interaction potential V (x) as follows V (x) = 0 for 0 x L ≤ ≤ = otherwise ∞ It is always a good idea to plot the potential energy, when it is a function of a single variable, as shown in Fig.1. The TISE is now given by V(x) V=infinity V=0 V=infinity x 0 L ~2 d2ψ(x) + V (x)ψ(x) = Eψ(x) −2m dx2 First consider the region outside the box where V (x) = .
    [Show full text]
  • The Quantum Mechanical Model of the Atom
    The Quantum Mechanical Model of the Atom Quantum Numbers In order to describe the probable location of electrons, they are assigned four numbers called quantum numbers. The quantum numbers of an electron are kind of like the electron’s “address”. No two electrons can be described by the exact same four quantum numbers. This is called The Pauli Exclusion Principle. • Principle quantum number: The principle quantum number describes which orbit the electron is in and therefore how much energy the electron has. - it is symbolized by the letter n. - positive whole numbers are assigned (not including 0): n=1, n=2, n=3 , etc - the higher the number, the further the orbit from the nucleus - the higher the number, the more energy the electron has (this is sort of like Bohr’s energy levels) - the orbits (energy levels) are also called shells • Angular momentum (azimuthal) quantum number: The azimuthal quantum number describes the sublevels (subshells) that occur in each of the levels (shells) described above. - it is symbolized by the letter l - positive whole number values including 0 are assigned: l = 0, l = 1, l = 2, etc. - each number represents the shape of a subshell: l = 0, represents an s subshell l = 1, represents a p subshell l = 2, represents a d subshell l = 3, represents an f subshell - the higher the number, the more complex the shape of the subshell. The picture below shows the shape of the s and p subshells: (notice the electron clouds) • Magnetic quantum number: All of the subshells described above (except s) have more than one orientation.
    [Show full text]
  • Magnetic Quantum Number: Describes the Orbital of the Subshell  Ms Or S - Spin Quantum Number: Describes the Spin QUANTUM NUMBER VALUES
    ST. LAWRENCE HIGH SCHOOL A JESUIT CHRISTIAN MINORITY INSTITUTION STUDY MATERIAL FOR CHEMISTRY (CLASS-11) TOPIC- STRUCTURE OF ATOM SUBTOPIC- QUANTUM NUMBERS PREPARED BY: MR. ARNAB PAUL CHOWDHURY SET NUMBER-03 DATE: 07.07.2020 ------------------------------------------------------------------------------------------------------------------------------- In chemistry and quantum physics, quantum numbers describe values of conserved quantities in the dynamics of a quantum system. In the case of electrons, the quantum numbers can be defined as "the sets of numerical values which give acceptable solutions to the Schrödinger wave equation for the hydrogen atom". How many quantum numbers exist? A quantum number is a value that is used when describing the energy levels available to atoms and molecules. An electron in an atom or ion has four quantum numbers to describe its state and yield solutions to the Schrödinger wave equation for the hydrogen atom. There are four quantum numbers: n - principal quantum number: describes the energy level ℓ - azimuthal or angular momentum quantum number: describes the subshell mℓ or m - magnetic quantum number: describes the orbital of the subshell ms or s - spin quantum number: describes the spin QUANTUM NUMBER VALUES According to the Pauli Exclusion Principle, no two electrons in an atom can have the same set of quantum numbers. Each quantum number is represented by either a half-integer or integer value. The principal quantum number is an integer that is the number of the electron's shell. The value is 1 or higher (never 0 or negative). The angular momentum quantum number is an integer that is the value of the electron's orbital (for example, s=0, p=1).
    [Show full text]
  • A Relativistic Electron in a Coulomb Potential
    A Relativistic Electron in a Coulomb Potential Alfred Whitehead Physics 518, Fall 2009 The Problem Solve the Dirac Equation for an electron in a Coulomb potential. Identify the conserved quantum numbers. Specify the degeneracies. Compare with solutions of the Schrödinger equation including relativistic and spin corrections. Approach My approach follows that taken by Dirac in [1] closely. A few modifications taken from [2] and [3] are included, particularly in regards to the final quantum numbers chosen. The general strategy is to first find a set of transformations which turn the Hamiltonian for the system into a form that depends only on the radial variables r and pr. Once this form is found, I solve it to find the energy eigenvalues and then discuss the energy spectrum. The Radial Dirac Equation We begin with the electromagnetic Hamiltonian q H = p − cρ ~σ · ~p − A~ + ρ mc2 (1) 0 1 c 3 with 2 0 0 1 0 3 6 0 0 0 1 7 ρ1 = 6 7 (2) 4 1 0 0 0 5 0 1 0 0 2 1 0 0 0 3 6 0 1 0 0 7 ρ3 = 6 7 (3) 4 0 0 −1 0 5 0 0 0 −1 1 2 0 1 0 0 3 2 0 −i 0 0 3 2 1 0 0 0 3 6 1 0 0 0 7 6 i 0 0 0 7 6 0 −1 0 0 7 ~σ = 6 7 ; 6 7 ; 6 7 (4) 4 0 0 0 1 5 4 0 0 0 −i 5 4 0 0 1 0 5 0 0 1 0 0 0 i 0 0 0 0 −1 We note that, for the Coulomb potential, we can set (using cgs units): Ze2 p = −eΦ = − o r A~ = 0 This leads us to this form for the Hamiltonian: −Ze2 H = − − cρ ~σ · ~p + ρ mc2 (5) r 1 3 We need to get equation 5 into a form which depends not on ~p, but only on the radial variables r and pr.
    [Show full text]
  • Higher Levels of the Transmon Qubit
    Higher Levels of the Transmon Qubit MASSACHUSETTS INSTITUTE OF TECHNirLOGY by AUG 15 2014 Samuel James Bader LIBRARIES Submitted to the Department of Physics in partial fulfillment of the requirements for the degree of Bachelor of Science in Physics at the MASSACHUSETTS INSTITUTE OF TECHNOLOGY June 2014 @ Samuel James Bader, MMXIV. All rights reserved. The author hereby grants to MIT permission to reproduce and to distribute publicly paper and electronic copies of this thesis document in whole or in part in any medium now known or hereafter created. Signature redacted Author........ .. ----.-....-....-....-....-.....-....-......... Department of Physics Signature redacted May 9, 201 I Certified by ... Terr P rlla(nd Professor of Electrical Engineering Signature redacted Thesis Supervisor Certified by ..... ..................... Simon Gustavsson Research Scientist Signature redacted Thesis Co-Supervisor Accepted by..... Professor Nergis Mavalvala Senior Thesis Coordinator, Department of Physics Higher Levels of the Transmon Qubit by Samuel James Bader Submitted to the Department of Physics on May 9, 2014, in partial fulfillment of the requirements for the degree of Bachelor of Science in Physics Abstract This thesis discusses recent experimental work in measuring the properties of higher levels in transmon qubit systems. The first part includes a thorough overview of transmon devices, explaining the principles of the device design, the transmon Hamiltonian, and general Cir- cuit Quantum Electrodynamics concepts and methodology. The second part discusses the experimental setup and methods employed in measuring the higher levels of these systems, and the details of the simulation used to explain and predict the properties of these levels. Thesis Supervisor: Terry P. Orlando Title: Professor of Electrical Engineering Thesis Supervisor: Simon Gustavsson Title: Research Scientist 3 4 Acknowledgments I would like to express my deepest gratitude to Dr.
    [Show full text]
  • The Principal Quantum Number the Azimuthal Quantum Number The
    To completely describe an electron in an atom, four quantum numbers are needed: energy (n), angular momentum (ℓ), magnetic moment (mℓ), and spin (ms). The Principal Quantum Number This quantum number describes the electron shell or energy level of an atom. The value of n ranges from 1 to the shell containing the outermost electron of that atom. For example, in caesium (Cs), the outermost valence electron is in the shell with energy level 6, so an electron incaesium can have an n value from 1 to 6. For particles in a time-independent potential, as per the Schrödinger equation, it also labels the nth eigen value of Hamiltonian (H). This number has a dependence only on the distance between the electron and the nucleus (i.e. the radial coordinate r). The average distance increases with n, thus quantum states with different principal quantum numbers are said to belong to different shells. The Azimuthal Quantum Number The angular or orbital quantum number, describes the sub-shell and gives the magnitude of the orbital angular momentum through the relation. ℓ = 0 is called an s orbital, ℓ = 1 a p orbital, ℓ = 2 a d orbital, and ℓ = 3 an f orbital. The value of ℓ ranges from 0 to n − 1 because the first p orbital (ℓ = 1) appears in the second electron shell (n = 2), the first d orbital (ℓ = 2) appears in the third shell (n = 3), and so on. This quantum number specifies the shape of an atomic orbital and strongly influences chemical bonds and bond angles.
    [Show full text]
  • Relativistic Quantum Mechanics 1
    Relativistic Quantum Mechanics 1 The aim of this chapter is to introduce a relativistic formalism which can be used to describe particles and their interactions. The emphasis 1.1 SpecialRelativity 1 is given to those elements of the formalism which can be carried on 1.2 One-particle states 7 to Relativistic Quantum Fields (RQF), which underpins the theoretical 1.3 The Klein–Gordon equation 9 framework of high energy particle physics. We begin with a brief summary of special relativity, concentrating on 1.4 The Diracequation 14 4-vectors and spinors. One-particle states and their Lorentz transforma- 1.5 Gaugesymmetry 30 tions follow, leading to the Klein–Gordon and the Dirac equations for Chaptersummary 36 probability amplitudes; i.e. Relativistic Quantum Mechanics (RQM). Readers who want to get to RQM quickly, without studying its foun- dation in special relativity can skip the first sections and start reading from the section 1.3. Intrinsic problems of RQM are discussed and a region of applicability of RQM is defined. Free particle wave functions are constructed and particle interactions are described using their probability currents. A gauge symmetry is introduced to derive a particle interaction with a classical gauge field. 1.1 Special Relativity Einstein’s special relativity is a necessary and fundamental part of any Albert Einstein 1879 - 1955 formalism of particle physics. We begin with its brief summary. For a full account, refer to specialized books, for example (1) or (2). The- ory oriented students with good mathematical background might want to consult books on groups and their representations, for example (3), followed by introductory books on RQM/RQF, for example (4).
    [Show full text]
  • The Extent of Acceptance of the Non-Separable Solution in Cylindrical Coordinates Through the Hydrogen Atom
    Advanced Studies in Theoretical Physics Vol. 13, 2019, no. 8, 433 - 437 HIKARI Ltd, www.m-hikari.com https://doi.org/10.12988/astp.2019.91246 The Extent of Acceptance of the Non-separable Solution in Cylindrical Coordinates through the Hydrogen Atom Mohammad F. Alshudifat Dept. of Physics, Al al-Bayt University, Mafraq 25113, Jordan This article is distributed under the Creative Commons by-nc-nd Attribution License. Copyright c 2019 Hikari Ltd. Abstract The hydrogen atom has been used to measure the extent of accep- tance of the non-separable solution in cylindrical coordinates. This work is not representing a new solution for the hydrogen atom, but to see how the non-separable solution in cylindrical coordinates gives acceptable results when compared with the known separable solution in spherical coordinates. The current work shows that the energy states (labeled by n = 1; 2; 3; :::) were found to be consistent with the Rutherford-Bohr model. The azimuthal quantum number ` was found to have a single value for each energy state, while the magnetic quantum number m was found to have two allowed values ` and ` − 1 for each energy state, this shrank the degeneracy of the excited states (n`m) to only two different states (n``) and (n` ` − 1), this result veers from the degeneracy cal- culated using spherical coordinates. A comparison between this work and the known solution in spherical coordinates show some acceptable results especially for the energy of atomic states, which is promising to use cylindrical coordinate in quantum problems when the spherical symmetry is deformed. Keywords: Cylindrical coordinates, non-separable solution, hydrogen atom, energy states, azimuthal quantum number, angular momentum 434 Mohammad F.
    [Show full text]