PHY331 Magnetism. Lecture 3

Similar documents
PHY331 Magnetism. Lecture 4

Solid State Physics MAGNETISM I. Lecture 27. A.H. Harker. Physics and Astronomy UCL

PHY331 Magnetism. Lecture 6

Electromagnetism - Lecture 10. Magnetic Materials

Magnetic materials, & inductance & Torque. P.Ravindran, PHY041: Electricity & Magnetism 8 February 2013: Magnetic materials, inductance, and torque

Lecture 5. Chapters 3 & 4. Induced magnetization: that which is induced in the presence of an applied magnetic field. diamagnetic.

Magnetic Materials. 2. Diamagnetism. Numan Akdoğan.

l μ M Right hand Screw rule

MSE 7025 Magnetic Materials (and Spintronics)

Electromagnetism II. Cristina Lazzeroni Lecture 5

Paramagnetism and Diamagnetism. Paramagnets (How do paramagnets differ fundamentally from ferromagnets?)

Physics of Magnetism. Chapter references are to Essentials of Paleomagnetism, UC Press, 2010

PHY331 Magnetism. Lecture 8

Physics 202, Lecture 14

Electromagnetism II. Instructor: Andrei Sirenko Spring 2013 Thursdays 1 pm 4 pm. Spring 2013, NJIT 1

2. When the current flowing through a wire loop is halved, its magnetic moment will become a. half. b. one-fourth. c. double. d. quadruple.

The magnetic circuits and fields in materials

Lecture 24 - Magnetism

Chemistry 431. Lecture 23

Solid state physics. Lecture 9: Magnetism. Prof. Dr. U. Pietsch

COPYRIGHTED MATERIAL. Production of Net Magnetization. Chapter 1

Physics 202, Lecture 14

CHAPTER 2 MAGNETISM. 2.1 Magnetic materials

( (Chapter 5)(Magnetism and Matter)

~~r ~o~/, ' , I. l: z: n.-b -z 01. ?;Cl. 60) Pro CD'fCJ7 '; ftu-0j~

Magnetism. March 10, 2014 Physics for Scientists & Engineers 2, Chapter 27 1

PHY331 Magnetism. Lecture 1

Def.: Magnetism the property of a material to be attracted to (paramagnetic response) or repelled by (diamagnetic response) a magnetic field

1 Magnetism, Curie s Law and the Bloch Equations

Ch. 28: Sources of Magnetic Fields

1. POLARIZATION AND MAGNETIZATION

μ (vector) = magnetic dipole moment (not to be confused with the permeability μ). Magnetism Electromagnetic Fields in a Solid

Magnetic Materials. 1. Magnetization 2. Potential and field of a magnetized object

Nuclear Magnetic Resonance Spectroscopy

Magnetic field and magnetic poles

Linear and Nonlinear Magnetic Media (Griffiths Chapter 6: Sections 3-4) Auxiliary Field H We write the total current density flowing through matter as

Lecture contents. Magnetic properties Diamagnetism Band paramagnetism Atomic paramagnetism Ferromagnetism. Molecular field theory Exchange interaction

Electromagnetism - Lecture 12. Ferromagnetism & Superconductivity

Luigi Paolasini

PHYSICS 4750 Physics of Modern Materials Chapter 8: Magnetic Materials

Sources of Magnetic Field

Section 24.8 Magnets and Magnetic Materials Pearson Education, Inc.

NMR Spectroscopy Laboratory Experiment Introduction. 2. Theory

Physics 1402: Lecture 17 Today s Agenda

Current Loop as a Magnetic Dipole & Dipole Moment:

Lecture 24 Origins of Magnetization (A number of illustrations in this lecture were generously provided by Prof. Geoffrey Beach)

Lecture 17. Magnetic Materials. Electromagnetic Induction. Faraday s Law

Magnetic Materials. The inductor Φ B = LI (Q = CV) = L I = N Φ. Power = VI = LI. Energy = Power dt = LIdI = 1 LI 2 = 1 NΦ B capacitor CV 2

The Oxford Solid State Basics

MR Fundamentals. 26 October Mitglied der Helmholtz-Gemeinschaft

Welcome back to PHYS 3305

physics 590 ruslan prozorov magnetic measurements Nov 9,

The Basics of Magnetic Resonance Imaging

12:40-2:40 3:00-4:00 PM

1. Aims. 2. Apparatus. 3. Background

Kirchhoff s rules, example

Chapter 5. Magnetism and Matter

Electricity & Optics

Magnetism and Levitation

Interaction of matter with magnetic fields

Physics 202, Lecture 14

Columbia University Department of Physics QUALIFYING EXAMINATION

Displacement Current. Ampere s law in the original form is valid only if any electric fields present are constant in time

Chapter 6. Magnetostatic Fields in Matter

Coaxial cable. Coaxial cable. Magnetic field inside a solenoid

ELECTRON SPIN RESONANCE & MAGNETIC RESONANCE TOMOGRAPHY

Statistical and Thermal Physics. Problem Set 5

Magnetic Field Lines for a Loop

Physics 1402: Lecture 18 Today s Agenda

Contour Plots Electron assignments and Configurations Screening by inner and common electrons Effective Nuclear Charge Slater s Rules

Magnetic Moments and Spin

Lecture 4; January Electrons in Atoms: Magnetism; Term Symbols, Z eff, and Other Properties

With that first concept in mind, it is seen that a spinning nucleus creates a magnetic field, like a bar magnet

Class XII Chapter 5 Magnetism And Matter Physics

NMR, the vector model and the relaxation

MAGNETIC EFFECTS OF CURRENT AND MAGNETISM

Let's look at the force on a current loop. In a uniform field it is zero: F = I I (dl B) =I I dl B =0 (4) since B is constant and comes outside the in

arxiv: v1 [physics.ed-ph] 22 Dec 2018

Magnetism and Magnetic Switching

Electron spin resonance

Types of Magnetism and Magnetic Domains

Ferromagnetism. In free space, the flux density and magnetizing field strength are related by the expression

Lecture B6 Molecular Orbital Theory. Sometimes it's good to be alone.

Towards understanding Precessional Motion

Class 11 : Magnetic materials

VIII. NUCLEAR MAGNETIC RESONANCE (NMR) SPECTROSCOPY

Electromagnetic fields Learning outcome

PHY481 - Lecture 29 Chapter 9 of PS, Chapters 6,7 of Griffiths

2 B B D (E) Paramagnetic Susceptibility. m s probability. A) Bound Electrons in Atoms

ψ s a ˆn a s b ˆn b ψ Hint: Because the state is spherically symmetric the answer can depend only on the angle between the two directions.

MAGNETIC MATERIALS. Fundamentals and device applications CAMBRIDGE UNIVERSITY PRESS NICOLA A. SPALDIN

Elements of magnetism and magnetic measurements

11/13/2018. The Hall Effect. The Hall Effect. The Hall Effect. Consider a magnetic field perpendicular to a flat, currentcarrying

Consider a magnetic field perpendicular to a flat, currentcarrying

Physics Sep Example A Spin System

Magnetism.

Outside the solenoid, the field lines are spread apart, and at any given distance from the axis, the field is weak.

Spin. Nuclear Spin Rules

Transition Elements. pranjoto utomo

Line spectrum (contd.) Bohr s Planetary Atom

Transcription:

PHY331 Magnetism Lecture 3

Last week Derived magnetic dipole moment of a circulating electron. Discussed motion of a magnetic dipole in a constant magnetic field. Showed that it precesses with a frequency called the Larmor precessional frequency

This week Discuss Langevin s theory of diamagnetism. Use angular momentum of precessing electron in magnetic field to derive the magnetization of a sample and thus diamagnetic susceptibility. Will set the scene for the calculation of paramagnetic susceptibility.

Langevin s theory of diamagnetism We want to calculate the sample magnetisation M and the diamagnetic susceptibility χ (recall M = χh) Every circulating electron on every atom has a magnetic dipole moment The sum of the magnetic dipole moments on any atom is zero (equal numbers circulating clockwise and anticlockwise?) The magnetisation M arises from the reaction to the torque Γ due to the applied magnetic field B which creates the Lamor precessional motion at frequency ω L.

i) the angular momentum L of the circulating electron is, L = mvr = mω r 2 The angular momentum L p of the precessional motion is, L p = mω L r 2 where ω L is the Larmor frequency and <r 2 > is the mean square distance from an axis through the nucleus which is parallel to B

ii) We showed last week that the magnetic moment m p per electron associated with L p is m p = e 2m L p so the total magnetisation M of the sample must be, M = N atoms Z electrons/atom m p M = N Z m p

So substitute for each quantity, in turn, M = N Z e 2m L p M = N Z e 2m mω L r 2 M = N Z e 2m m eb r 2 2m so that, χ = M H = µ 0N Z e2 4m r 2

Now express <r 2 > in terms of the mean square radius of the orbit <ρ 2 >, where will give r 2 = 2 3 ρ 2 χ = µ 0 N Z e2 6m ρ 2 ρ 2 = x 2 + y 2 + z 2 x 2 = y 2 = z 2 = ρ 2 /3 r 2 = x 2 + y 2 The result we wanted!!

What does this mean??? The atom as a whole does not possess a permanent magnetic dipole moment. The magnetisation is produced by the influence of the external magnetic field on the electron orbits and particularly by the precessional motion. The diamagnetic susceptibility χ is small and negative, because <ρ 2 > is small. Negative susceptability means that diamagnetism opposes applied magnetic field. (prefix: dia - in opposite or different directions) Note that measurements of χ were once used to get estimates of atomic size through the values of <ρ 2 >. Remember - all materials are diamagnetic but this small effect is swamped if also paramagnetic of ferromagnetic.

Paramagnetism Paramagnets have a small positive magnetisation M (directed parallel the applied field B). Each atom has a permanent magnetic dipole moment. Langevin (classical) theory The paramagnet consists of an array of permanent magnetic dipoles m In a uniform field B they have Potential Energy = - m.b

A dipole parallel to the field has the lowest energy BUT, the B field causes precession of m about B. However it can t alter the angle between m and B (as the L z component is constant in the precession equations). For the dipole to lower its energy (and become parallel to the field) we need a second mechanism. This is provided by the thermal vibrations The magnetic field would like the dipoles aligned to lower their energy The thermal vibrations would like to randomise and disorder the magnetic dipoles

We can therefore expect a statistical theory, based on a competition between these two mechanisms, k B T m.b to calculate the magnetisation M of a paramagnet

Calculate the magnetisation M of a paramagnet M must be the vector sum of all the magnetic dipole moments M = [1] Resolved component X of a dipole in field direction [2] Number of dipoles with this orientation To do this, use Boltzmann statistics to obtain the number dn of dipoles with energy between E and E + de ( ) de dn = c exp E kt where k = Boltzmann s constant, c = is a constant of the system and T = T measured in Kelvin

How to find c? Integrate over all the energies, which must give N the total number of dipoles N = 0 c exp ( E kt) de Next week we will do this to calculate the susceptibility of a paramagnet. The important result we will get will be That susceptibility is temperature dependent with χ = C/T This is Curie s law.

Summary Calculated the susceptibility for a diamagnet χ = µ 0 N Z e2 6m ρ 2 Argued that all materials have a small diamagnetic susceptibility resulting from the precession of electrons in a magnetic field. This precession results in a magnetic moment, and thus a susceptibility. Then discussed paramagnetism, resulting from atoms having a permanent magnetic moment. Sketched out how we will calculate paramagnetic susceptibility.