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Magnetic Properties

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The magnetic moment due to the precession is mp=-(e/2m) Lp. Total magnetization of a sample: ... Precession cannot change the angle between B and m ... – PowerPoint PPT presentation

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Title: Magnetic Properties


1
Magnetic Properties
  • Subhalakshmi Lamba

2
Langevins Theory of Diamagnetism
i
e
Magnetic Dipole moment of an electron in an
atomic orbit ??
3
Langevins Theory of Diamagnetism
electron
r
Nucleus
d A
d l
4
Langevins Theory of Diamagnetism
ANGULAR MOMENTUM
5
Langevins Theory of Diamagnetism
  • What happens to the magnetic dipole moment of the
    circulating electron in a constant magnetic
    field?
  • The field produces a torque ? m ? B on each
    dipole
  • Purely precessional motion

6
Larmor Precession
  • Frequency of precession Larmor frequency ?p
  • Angular momentum
  • L p m ?p lt r2gt
  • (eB/2) lt r2gt

e
L
?peB/2m
7
Langevins Theory of Diamagnetism
  • The magnetic moment due to the precession is
    mp-(e/2m) Lp.
  • Total magnetization of a sample
  • (No. of atoms) ? (No. of electrons/atom) ? mp

8
Langevins Theory of Diamagnetism
  • M - N Z (e/2m) Lp.
  • M - N Z (e/2m) (eB/2) lt r2gt B ?0H
  • ? M/H - ?0N Z (e2/4m). lt r2gt

9
Finding ltr2gt
  • lt r2gt is the mean square distance of the
    electron from the axis through the nucleus and
    parallel to the field

Z
  • Mean square
  • radius of the
  • electron orbit

r2x2y2
Y
r
X
?2x2y2z2
10
Finding ltr2gt
  • ltx2gtlty2gtltz2gt(1/3) lt?2gt for a spherically
    symmetric charge distribution
  • ltr2gtltx2gtlty2gt(2/3) lt?2gt
  • ? - ?0N Z (e2/6m). lt?2gt

11
The diamagnetic susceptibility
  • is negative
  • does not depend on temperature
  • Is very small because lt?2gt is very small
  • is a property of all matter

12
Merit of the Theory
  • Langevins theory explains for all the major
    properties of diamagnetic materials
  • The atom as a whole does not have a permanent
    magnetic moment
  • Magnetization is produced by the effect of the
    externally applied magnetic field on the
    circulating electron

13
PARAMAGNETISM
  • Each atom has a permanent magnetic dipole moment
  • Each dipole has an energy of m.B
  • which is m B cos ??
  • Energy is minimum when m is parallel to B

?
14
Two mechanisms at work
  • Effect of the field is to cause a precession of
    the magnetic moment about the field.
  • Precession cannot change the angle between B and
    m
  • How do the magnets align to the external field?

Thermal vibrations
15
Two mechanisms at work
The magnetic field tends to align the dipole
Thermal vibrations tend to randomize the dipoles
  • Statistical Theory

Total Magnetization ?? (component of the dipole
moment in the direction of the field) X (No. of
dipoles which have this orientation wrt the field)
16
A classical theory for Paramagnetism
Component of the dipole in the direction of the
field is m cos ?
Energy E -m B cos ?
?
dE m B sin ? d ?
17
A classical theory for Paramagnetism
No of dipoles which have an energy between E and
E dE No. of dipoles which have an orientation
between ? and d?
dn c exp(-E/kBT) dE c
exp(mBcos?/kBT)m B sin? d?
18
A classical theory for Paramagnetism
19
A classical theory for Paramagnetism
  • A parameter which is a measure of the ratio of
    the two competing energies

20
A classical theory for Paramagnetism
LANGEVIN FUNCTION L(a)
21
A classical theory for Paramagnetism
L(a)
a
PAUL LANGEVIN
22
A classical theory for Paramagnetism
Magnetization of a paramagnetic substance M N
m L(a) amB/kBT ? M/H
23
At the limits
  • At small applied fields and high temperatures T
  • a is small

24
At the limits
CURIES LAW
25
At the limits
  • Large applied field B compared to the
    temperature T
  • a is small

26
At the limits
SATURATION maximum possible magnetization Magnet
ization becomes independent of the applied field
27
A RECAP
  • Classical Theory of Magnetism
  • Circulating Electron magnetic dipole of the
    atom
  • Diamagnetism due to the effect of the external
    magnetic field on the magnetic dipole moment.
  • A weak effect depends on atomic radius, which
    is very small

28
A RECAP
  • Paramagnetism competitiion between the magnetic
    field and temperature
  • Alignment to the field versus randomization
  • Statistical Treatment
  • Saturation at high fields
  • Curies law for low fields

29
NEED for a Quantum Theory
  • Niels Bohr 1911, and J.H van Leeuwen
    independently in 1919 in her PhD thesis proved a
    famous theorem for classical nonrelativistic
    electrons using Maxwell's equations and
    statistical mechanics
  • "At any finite temperature, and in all finite
    applied electrical or magnetic fields, the net
    magnetization of a collection of electrons in
    thermal equilibrium vanishes identically."

30
NEED for a Quantum Theory
  • Classical Physics cannot give any kind of
    magnetism
  • Explanation for ferromagnetism Pauli principle
    that no two electrons could occupy the same
    state. Together with the Coulomb interaction
    between electrons, this leads to a scalar
    isotropic interaction of two spins with a
    positive exchange constant J.
  • Physical explanation for the Molecular fields of
    Weiss

31
NEED for a Quantum Theory
  • Zeeman Effect offered experimental support for
    the quantization of angular momentum

32
NEED for a Quantum Theory
  • Anomalous Zeeman Effect the magnetic field
    split the lines into four, six, or even more
    lines and some triplets showed wider spacings
    than expected
  • Only explained by including electron spin
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