Non-Relativistic > s.a. classical
systems; mass; particle
models; spinning
particles.
* Action: Of the form
S[xi; t1, t2]
=
12
dt [
m
i (x·i)2– V(xi)]
.
@ Various backgrounds: Baleanu & Güler JPA(01)ht [in
curved spacetime, Hamilton-Jacobi]; Chavchanidze & Tskipuri
mp/01 [SU(2)
group]; Marques & Bezerra CQG(02)gq/01 [cosmic
string].
@ Symmetries: Haas & Goedert JPA(99)mp/02 [2D,
Noether]; Jahn & Sreedhar AJP(01)mp [invariance
group].
@ Related topics: Fuenmayor et al PRD(02)ht/01 [loop
representation, with gauge theory]; van Holten phy/01 [dual
fluid interpretation].
@ Variations: Barbour CQG(03)gq/02 [relational dynamics]; > s.a. parametrized
theories.
Relativistic Particles > s.a. self-force; test-body orbits.
$ Action, reparametrization-invariant:
Two
versions, which give the trajectory
only as
a locus of points,
are
S[x] = m0c
ds |gab x·a x·b|1/2 =
dt (pa x·a –
g p2) or S[x]
=
dt (u–1 gab x·a x·b –
um2) ;
The first one (Jacobi-type) is proportional
to the length of the world-line, the g(t) is a 1D metric/Lagrange
multiplier, like 1D gravity with scalars, and u(t) is an additional variable.
$ Action, proper-time-gauge:
S[x] =
m0
dt gab x·a x·b .
* Equation of motion:
If a particle is coupled to a field, its equation of motion is just the expression
of momentum exchange
between particle and field, so it can be obtained
from
a Ttotab =
0; For a scalar particle in electromagnetic field and linearized
gravity, respectively,
dpm/d
= q Fmn un
= (q/m) Fmn pn
, dpm/d
=
(
/2)
m hab,m uaub
.
* Issue: The descriptions using t and the proper time
are
not equivalent [@ Kalman PR(61); Sonego PRA(91)].
* Issue: If a point particle
is included among the field sources, the treatment cannot be made fully consistent.
@ Lagrangian formulation: Potgieter AJP(83),
comment Berger AJP(84);
Desloge & Eriksen AJP(85).
@ In curved spacetime: Modanese JMP(92)
[fluctuating gravitational field]; Piechocki CQG(03)gq/02 [dS,
different topologies]; Bini et al
CQG(03)gq/02 [in
gravitational wave collision]; Barrabès & Hogan
CQG(04)gq/03 [deflection];
Chicone & Mashhoon CQG(05)gq/04 [in
Fermi coordinates]; Fukumoto et al PTP(06)gq [finite-size,
fast-moving]; Ling et al gq/06 [in
rainbow spacetime]; > s.a. kerr-newman, scattering.
@ Interacting: Bergmann & Komar GRG(82); Tretyak & Nazarenko
CondMP(00)ht; Damour
et al PLB(01)gq [3PN];
Lompay ht/05.
@ Stochastic
medium:
Johnson & Hu PRD(02)
[modified Abraham-Lorentz-Dirac equation in a quantum field]; Cabo-Bizet & Cabo
Montes de Oca PLA(06).
@ Related topics: Balachandran et al JMP(84)
[geometry]; Gill et al IJTP(93),
IJTP(98)
[proper time formulation]; Horwitz ht/98 [Lorentz force equation from Stückelberg
mechanics]; Parrott gq/02 [Rohrlich
equation]; Barros et al
CQG(05)
[with rigidity and torsion]; Uggerhøj RMP(05)
[in strong crystalline fields]; Freidel et al PRD(07)
[Dirac observables and effective noncommutative geometry].
> Other topics: see mass; non-commutative
physics; radiation; scalar
field theories; specific heat; statistical
mechanics; Test
Body.
Variations and Generalizations > s.a. dissipative
system; quantum particles [including superparticle]; spinning
particles.
$ Charged particle:
The length-of-worldline action becomes
S[x] =
ds [m0c |gab x·a x·b|1/2 + q Aa x·a]
.
* Modified
Lagrangian: It can depend on the curvature of the worldline (rigidity)
and its torsion.
@ Charged particle: Hyman
AJP(97), Muñoz AJP(97)
[with constant fields];
Aldaya et al JPA(02)
[group cohomology]; Cardoso et al PRD(03)
[in Schwarzschild]; Carvalho et al IJMPA(04)gq [with
defect distribution]; Timoumi RPMP(04)
[closed trajectories]; Lidsky TMP(05)
[radiating]; Rohrlich 07; > s.a. self-force [including
preacceleration]; Marmo & Tulczyjew RPMP(06)
[Poincaré-covariant, and T reflection]; > s.a. electromagnetism.
@ Alternative dynamics: Arreaga et al CQG(01)ht [Frenet-Serrat
curvature action]; Pavón JMP(01)qp [stochastic
dynamics].
Coupled to Gravity > s.a. 3D
gravity; multipoles [extended
objects]; orbits; quantum
particles; radiation; spinning
particles; Test
Body.
@ Non-spinning: Kaniel & Itin gq/01; Blanchet & Faye JMP(01)gq/00 [regularization].
@ Charged: Rosen AP(62) [field of particle in motion]; Khriplovich & Pomeransky gq/98-in;
Khriplovich
ht/00-in
[spinning]; Das et al mp/05 [review];
Gorbatenko TMP(05)
[Einstein-Infeld-Hoffmann, order (v/c)3].
@ With torsion: Fiziev & Kleinert gq/96 [action];
Kleinert & Pelster
GRG(99)gq/96 [autoparallels];
Barros e Sá gq/97;
Geyer et al IJMPA(00)ht/99;
Pezzaglia gq/99/IJTP;
Arroyo et al GRG(04)ht/03;
Barros et al IJMPA(04).
Main page – Abbreviations – Journals – Comments – Other
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Send feedback and suggestions to bombelli at olemiss.edu – Modified
25 may 2008