Effects In General > s.a. nuclear
physics [fusion]; superconductivity.
* Barnett effect: The
magnetization of a rotating body, discovered in
1915
by S J Barnett; > s.a. gravitomagnetism.
* Larmor frequency: The precession frequency of a magnetic dipole in
a uniform magnetic field; Example: For a particle with classical gyromagnetic
ratio
=
q/2mc, its value is
L = –qB/2mc.
* Maximum value: According
to a QED calculation of the effect of a magnetic field on positronium, the maximum
magnetic field is 1042 G, since at a higher
value "the vacuum would explode by producing collapsed positronia".
* Magnetic cooling: A.k.a.
magnetocaloric effect,
the cooling caused by heat absorption by previously aligned magnetic nuclei when
the external magnetic field is removed.
@ General references: Farley & Price AJP(01)
[long, finite solenoid]; Jancewicz & Brzeski EJP(05)
[magnetic field surfaces]; Shabad & Usov PRL(06)
+ pw(06)may
[maximum
value]; Labinac et al AJP(06)
[cylindrical coil].
@ Effects on charges: Gascón & Peralta-Salas PLA(04) [impossibility
of
reaching source wires]; Rousseaux phy/05 [j
A interaction]; > s.a. quantum
systems.
> Other effects:
see Bohr Magneton; Hall
Effect; quantum measurement.
In Astrophysics and Cosmology > s.a. contents
of the universe; galaxies [including Milky
Way]; galaxy evolution; neutron
stars.
* Milky Way: The
magnetic field in Stanev's model is parametrized as
BMW = (3R/r)
cos(
–
ln r/r0)
exp{–z/z0} (not
that good near galactic center).
* Interstellar: One
way to detect a B field in interstellar space is to look for polarization
of starlight passing through it.
@ Reviews: Maartens Pra(00)ap;
Han ASS(01)ap/00-in
[Milky Way].
@ Estimates: Anchordoqui & Goldberg PRD(02)hp/01 [local
intergalactic B > 10–8 G];
Clarkson et al CQG(03)ap/02 [bounds
from cmb]; Ferretti & Johnston-Hollitt ap/04-in,
Ensslin et al ap/05-in
[galaxy clusters]; Opher et al Sci(07)may-a0705 [local
interstellar].
@ Primordial: Garretson et al PRD(92)hp;
Field & Carroll PRD(00);
Durrer & Caprini JCAP(03)
[and causality]; news pw(06)jan
[origin].; de Souza & Opher ap/06 [origin
in electromagnetic fluctuations]; Durrer ap/06-in,
Yamazaki et al ApJ(06)ap, ap/06-in
[and cmb]; Yamazaki et al PRD(06)ap [and
large-scale structure]; Battefeld et al a0708 [cosmic
string loops]; > s.a. modified electromagnetism.
@ And inflation: Giovannini & Shaposhnikov PRD(00);
Bamba & Sasaki JCAP(07)ap/06.
@ Origin: Widrow RMP(02)ap/02;
Gaensler et al NAR(04)ap;
Dar & De Rújula PRD(05)
[winds and cosmic rays]; Subramanian a0802-in.
Gravitation-Related > see black holes and black hole phenomenology; cosmological perturbations; duality [dual-magnetic mass]; gravitomagnetism; matter in cosmology; tests of general relativity [gravity of magnetic fields]; weyl tensor.
Other Phenomenology > s.a. magnetism [in matter, plasma physics].
@ References: Erlichson AJP(89), AJP(98)
[Biot-Savart experiment]; Duncan ap/00-in
[physics of very high B's]; > s.a. qed
phenomenology.
Main page – Abbreviations – Journals – Comments – Other
sites – Acknowledgements
Send feedback and suggestions to bombelli at olemiss.edu – Modified
14 jun 2008