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Origin of Magnetic Moment
Magnetism arises from the Magnetic Moment or Magnetic dipole of
Magnetic Materials.
When the electrons revolves around the nucleus Orbital magnetic
moment arises, similarly when the electron spins, spin Magnetic
moment arises.
The permanent Magnetic Moments can arise due to the
1.The orbital magnetic moment of the electrons
2.The spin magnetic moment of the electrons, and
3.The spin magnetic moment of the nucleus
Origin of magnetic dipoles
➒ The spin of the electron produces a magnetic field with a
direction dependent on the quantum number ml.
The spin of the electron produces a magnetic field with
a direction dependent on the quantum number ms.
Origin of magnetic dipoles
Electrons orbiting around the nucleus create a magnetic
field around the atom.
➒ Materials can be classified based on their magnetic property or behavior
β€’ magnetic susceptibility πœ’π‘š
β€’ relative permeability πœ‡π‘Ÿ
➒ A material is said to be nonmagnetic if πœ’π‘š = 0 or πœ‡π‘Ÿ = 1; it is magnetic
otherwise.
➒ Free space, air, and materials with πœ’π‘š = 0 or πœ‡π‘Ÿ β‰ˆ 1 are regarded as
nonmagnetic.
➒ Materials may be grouped into three major classes:
β€’ diamagnetic
β€’ paramagnetic and
β€’ ferromagnetic
Diamagnetic Materials
β€’ It is a weak form of magnetism
β€’ Diamagnetism is because of orbital magnetic moment.
β€’ No permanent dipoles are present so net magnetic moment is zero.
β€’ Persists only when external field is applied.
β€’ Dipoles are induced by change in orbital motion of electrons due to applied magnetic field.
β€’ Diamagnetic susceptibility is independent of temperature and applied magnetic field strength.
β€’ Susceptibility is of the order of -10-5.
β€’ Relative permeability is less than one.
β€’ It is present in all materials, but since it is so weak it can be observed only when other types of
magnetism are totally absent.
β€’ Examples: Bi, Zn, gold, H2O, alkali earth elements (Be, Mg, Ca, Sr), superconducting
elements in superconducting state.
No Applied
Magnetic Field (H = 0)
Applied
Magnetic Field (H)
none
opposing
Paramagnetic Materials
β€’ Possess permanent dipoles.
β€’ If the orbital's are not completely filled or spins not balanced, an overall small magnetic
moment may exist. (i.e.) paramagnetism is because of orbital and spin magnetic
moments of the electron.
β€’ In the absence of external magnetic field
β€’ all dipoles are randomly oriented
β€’ so net magnetic moment is zero.
β€’ In presence of magnetic field the material gets feebly magnetized i.e. the material allows
few magnetic lines of force to pass through it.
β€’ Relative permeability Β΅r >1 (barely, β‰ˆ 1.00001 to 1.01).
β€’ The orientation of magnetic dipoles depends on temperature and applied field.
β€’ Susceptibility is independent of applied mag. field & depends on temperature
β€’ Susceptibility is small and positive.
β€’ The susceptibility range from 10-5 to 10-2.
β€’ Examples: alkali metals (Li, Na, K, Rb), transition metals, Al, Pt, Mn, Cr etc.
No Applied
Magnetic Field (H = 0)
Applied
Magnetic Field (H)
random
aligned
Paramagnetic Materials
Ferromagnetic Materials
β€’ Permanent dipoles are present so possess net magnetic moment
β€’ Origin for magnetism in Ferro mag. Materials is due to Spin magnetic moment of
electrons.
β€’ Material shows magnetic properties even in the absence of external magnetic field.
β€’ Possess spontaneous magnetization.
β€’ Spontaneous magnetization is because of interaction between dipoles called
EXCHANGE COUPLING.
β€’ When placed in external mag. field it strongly attracts magnetic lines of force.
β€’ All spins are aligned parallel & in same direction.
β€’ Susceptibility is large and positive, it is given by Curie Weiss Law
β€’ Material gets divided into small regions called domains.
β€’ They possess the property of HYSTERESIS.
β€’ Examples: Fe, Co, Ni.
aligned
aligned
No Applied
Magnetic Field (H = 0)
Applied
Magnetic Field (H)
Ferromagnetic Materials
MAGNETIC BOUNDARY CONDITIONS
β€’ We define magnetic boundary conditions as the conditions that H (or B) field must satisfy
at the boundary between two different media.
β€’ By Gauss’s law for magnetic fields
β†’ 1
β€’ Consider the boundary between two magnetic media 1 and 2, characterized, respectively,
by and πœ‡1 and πœ‡2 as in Figure.
β€’ Applying eq. 1 to the pillbox (Gaussian surface) for the above Figure and allowing
Ξ”β„Ž β†’ 0, we obtain
𝐁 = πœ‡ 𝐇
β€’ If the boundary is free of current or the media are not conductors (for K is free current
density), K = 0 and eq. 3 becomes
β€’ Thus the tangential component of H is continuous while that of B is discontinuous at the
β€’ boundary.
β€’ If the fields make an angle πœƒ with the normal to the interface, we get,
πΆπ‘œπ‘ πœƒ1 =
B1𝑛
B1
⟹ B1 πΆπ‘œπ‘ πœƒ1 = B1𝑛
Similarly πΆπ‘œπ‘ πœƒ2 =
B2𝑛
B2
⟹ B2 πΆπ‘œπ‘ πœƒ2 = B2𝑛
1
and π‘†π‘–π‘›πœƒ1 =
H1𝑑
H1
⟹ H1 π‘†π‘–π‘›πœƒ1 = H1𝑑
⟹
𝐡1
πœ‡1
π‘†π‘–π‘›πœƒ1 = H1𝑑
and π‘†π‘–π‘›πœƒ2 =
H2𝑑
H2
⟹ H2 π‘†π‘–π‘›πœƒ2 = H2𝑑
⟹
𝐡2
πœ‡2
π‘†π‘–π‘›πœƒ2 = H2𝑑
⟹
𝐡1
πœ‡1
π‘†π‘–π‘›πœƒ1 = H1𝑑
2
Dividing equ. 2 by equ. 1 we get
⟹
tan πœƒ1
tan πœƒ2
=
πœ‡1
πœ‡2
tan πœƒ1
πœ‡1
=
tan πœƒ2
πœ‡2

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EMF 4.pdf

  • 1. Origin of Magnetic Moment Magnetism arises from the Magnetic Moment or Magnetic dipole of Magnetic Materials. When the electrons revolves around the nucleus Orbital magnetic moment arises, similarly when the electron spins, spin Magnetic moment arises. The permanent Magnetic Moments can arise due to the 1.The orbital magnetic moment of the electrons 2.The spin magnetic moment of the electrons, and 3.The spin magnetic moment of the nucleus
  • 2. Origin of magnetic dipoles ➒ The spin of the electron produces a magnetic field with a direction dependent on the quantum number ml.
  • 3. The spin of the electron produces a magnetic field with a direction dependent on the quantum number ms. Origin of magnetic dipoles
  • 4. Electrons orbiting around the nucleus create a magnetic field around the atom.
  • 5. ➒ Materials can be classified based on their magnetic property or behavior β€’ magnetic susceptibility πœ’π‘š β€’ relative permeability πœ‡π‘Ÿ ➒ A material is said to be nonmagnetic if πœ’π‘š = 0 or πœ‡π‘Ÿ = 1; it is magnetic otherwise. ➒ Free space, air, and materials with πœ’π‘š = 0 or πœ‡π‘Ÿ β‰ˆ 1 are regarded as nonmagnetic. ➒ Materials may be grouped into three major classes: β€’ diamagnetic β€’ paramagnetic and β€’ ferromagnetic
  • 6.
  • 7. Diamagnetic Materials β€’ It is a weak form of magnetism β€’ Diamagnetism is because of orbital magnetic moment. β€’ No permanent dipoles are present so net magnetic moment is zero. β€’ Persists only when external field is applied. β€’ Dipoles are induced by change in orbital motion of electrons due to applied magnetic field. β€’ Diamagnetic susceptibility is independent of temperature and applied magnetic field strength. β€’ Susceptibility is of the order of -10-5. β€’ Relative permeability is less than one. β€’ It is present in all materials, but since it is so weak it can be observed only when other types of magnetism are totally absent. β€’ Examples: Bi, Zn, gold, H2O, alkali earth elements (Be, Mg, Ca, Sr), superconducting elements in superconducting state.
  • 8. No Applied Magnetic Field (H = 0) Applied Magnetic Field (H) none opposing
  • 9. Paramagnetic Materials β€’ Possess permanent dipoles. β€’ If the orbital's are not completely filled or spins not balanced, an overall small magnetic moment may exist. (i.e.) paramagnetism is because of orbital and spin magnetic moments of the electron. β€’ In the absence of external magnetic field β€’ all dipoles are randomly oriented β€’ so net magnetic moment is zero. β€’ In presence of magnetic field the material gets feebly magnetized i.e. the material allows few magnetic lines of force to pass through it. β€’ Relative permeability Β΅r >1 (barely, β‰ˆ 1.00001 to 1.01). β€’ The orientation of magnetic dipoles depends on temperature and applied field. β€’ Susceptibility is independent of applied mag. field & depends on temperature β€’ Susceptibility is small and positive. β€’ The susceptibility range from 10-5 to 10-2. β€’ Examples: alkali metals (Li, Na, K, Rb), transition metals, Al, Pt, Mn, Cr etc.
  • 10. No Applied Magnetic Field (H = 0) Applied Magnetic Field (H) random aligned Paramagnetic Materials
  • 11. Ferromagnetic Materials β€’ Permanent dipoles are present so possess net magnetic moment β€’ Origin for magnetism in Ferro mag. Materials is due to Spin magnetic moment of electrons. β€’ Material shows magnetic properties even in the absence of external magnetic field. β€’ Possess spontaneous magnetization. β€’ Spontaneous magnetization is because of interaction between dipoles called EXCHANGE COUPLING. β€’ When placed in external mag. field it strongly attracts magnetic lines of force. β€’ All spins are aligned parallel & in same direction. β€’ Susceptibility is large and positive, it is given by Curie Weiss Law β€’ Material gets divided into small regions called domains. β€’ They possess the property of HYSTERESIS. β€’ Examples: Fe, Co, Ni.
  • 12. aligned aligned No Applied Magnetic Field (H = 0) Applied Magnetic Field (H) Ferromagnetic Materials
  • 13.
  • 14.
  • 15. MAGNETIC BOUNDARY CONDITIONS β€’ We define magnetic boundary conditions as the conditions that H (or B) field must satisfy at the boundary between two different media. β€’ By Gauss’s law for magnetic fields β†’ 1
  • 16. β€’ Consider the boundary between two magnetic media 1 and 2, characterized, respectively, by and πœ‡1 and πœ‡2 as in Figure.
  • 17.
  • 18. β€’ Applying eq. 1 to the pillbox (Gaussian surface) for the above Figure and allowing Ξ”β„Ž β†’ 0, we obtain 𝐁 = πœ‡ 𝐇
  • 19.
  • 20. β€’ If the boundary is free of current or the media are not conductors (for K is free current density), K = 0 and eq. 3 becomes β€’ Thus the tangential component of H is continuous while that of B is discontinuous at the β€’ boundary. β€’ If the fields make an angle πœƒ with the normal to the interface, we get, πΆπ‘œπ‘ πœƒ1 = B1𝑛 B1 ⟹ B1 πΆπ‘œπ‘ πœƒ1 = B1𝑛 Similarly πΆπ‘œπ‘ πœƒ2 = B2𝑛 B2 ⟹ B2 πΆπ‘œπ‘ πœƒ2 = B2𝑛 1
  • 21. and π‘†π‘–π‘›πœƒ1 = H1𝑑 H1 ⟹ H1 π‘†π‘–π‘›πœƒ1 = H1𝑑 ⟹ 𝐡1 πœ‡1 π‘†π‘–π‘›πœƒ1 = H1𝑑 and π‘†π‘–π‘›πœƒ2 = H2𝑑 H2 ⟹ H2 π‘†π‘–π‘›πœƒ2 = H2𝑑 ⟹ 𝐡2 πœ‡2 π‘†π‘–π‘›πœƒ2 = H2𝑑 ⟹ 𝐡1 πœ‡1 π‘†π‘–π‘›πœƒ1 = H1𝑑 2 Dividing equ. 2 by equ. 1 we get ⟹ tan πœƒ1 tan πœƒ2 = πœ‡1 πœ‡2 tan πœƒ1 πœ‡1 = tan πœƒ2 πœ‡2