In General > s.a. aharonov-bohm
effect; dark
matter.
* Idea: The lens-like
effect produced by the deflection of waves (especially light) along different
paths.
* Remark: They are not linear lenses, and are not described by Gaussian
optics, but can use Fermat's principle.
* Theoretical results:
There is always an odd number of images, unless they are formed by a black
hole; Has enriched the field of geometrical optics.
* Experimental results:
VLA surveys yield few lenses; the universe cannot be closed by masses of 1011–1012 MSun;
They allow us to make
spectra of distant (z > 2) galaxies, because of amplification (they
are like 100-Kpc telescopes); Many double images of galaxies (some with opposite
parity) have been seen; The first complete Einstein ring has been seen, and
the (extended)
source object reconstructed.
* Future: Look for cosmic strings with the space telescope; dark matter.
In Specific Spacetimes > s.a. observational
cosmology; gravitational
wave propagation; tests of general relativity
with light.
@ By black holes: Virbhadra & Ellis PRD(00)ap/99 [Schwarzschild];
Eiroa et al PRD(02)gq [RN];
Vázquez & Esteban NCB(04)gq/03
[Kerr]; Whisker PRD(05)ap/04 [brane
world]; Eiroa PRD(06)
[Einstein-Born-Infeld]; Konoplya PLB(07)
[magnetized]; Sereno PRD(08)
[with cosmological constant, Schwarzschild-de Sitter].
@ By wormholes: Eiroa et al MPLA(01)gq,
Torres et al MPLA(01)gq [chromaticity];
Safonova et al PRD(02)gq/01;
Shatskiy AR(04)ap;
Tejeiro & Larrañaga gq/05;
Nandi et al PRD(06)gq; > s.a. wormholes.
@ Other isolated objects: Virbhadra & Ellis PRD(02)
[naked singularity]; Lake PRD(02)gq/01,
a0711 [with cosmological
constant]; Palle APS(05)ap [quadrupole
potentials]; Amore et al PRD(07)
[compact objects]; Park a0804 [with
cosmological constant].
@ Cosmic strings: de Laix PRD(97),
et al PRL(97);
Bernardeau & Uzan PRD(01)ap/00,
ap/00-in;
Shlaer & Tye PRD(05)
[and instability of closed timelike curves]; Agol et al PRD(06)
[HST candidate excluded]; Gasparini et al a0710-MNRAS; > s.a.
tests of general relativity with light [conical
defects].
@ Gravitational waves: Mollerach PRD(98)ap/97; Faraoni IJMPD(98), & Gunzig
A&A(98)ap [scalar-tensor].
@ Cosmological models: Wambsganss et al ap/96/ApJ;
Kaiser ApJ(98)ap/96.
@ Inhomogeneous, cumulative: Holz & Wald PRD(98)ap/97,
Wald gq/98-in [statistical distribution]; Bergstrom et al ap/99/A&A;
Claudel PRS(00)gq [including
swiss cheese]; Jain et al PRD(02)ap [brane
world]; > s.a. relativistic cosmology [local
models].
@ Related topics: Zaldarriaga PRD(00)ap/99 [and
cmb]; Safonova et al MPLA(01)ap [violations
of energy conditions].
Microlensing > s.a. cosmic
strings; dark
matter.
* Idea: Gravitational lensing by small objects.
* History: 1936, Paper by Einstein & other guy; 1986, Paczynski
proposed use for dark matter detection; 1999, Planet around a binary system
found with
it.
@ Reviews: Paczynski & Wambsganss PW(93);
Evans ap/96-in;
Gould ap/96-in, ap/00-in;
Roulet & Mollerach PRP(97);
Mao ap/99-in;
Paczynski
ap/99-in;
Sackett ap/00-in;
Evans ap/03-in;
Paczynski ap/03 [and
future]; Rattenbury MPLA(06)
[planetary]; Zakharov ap/06-in;
Gould a0803-in.
@ Theory, formalism: Gould ap/00/ApJ;
Asada ApJ(02)ap [perturbative].
@ Of gravitational waves: Bar-Kana PRD(96)ap [limits
on background]; De Paolis et al A&A(01)ap/00.
@ Related topics: Gould ap/96-in
[imaging binaries, quasars]; Jetzer HPA(96)ap, ap/97-in
[dark matter search]; MACHO collab ap/97-in
[data]; Paczynski ap/97/ApJL
[SIM plans]; Han et
al MNRAS(00)ap/99,
ApJ(04)ap/03 [free-floating
planets]; Smith et al MNRAS(03)ap/02 [acceleration
and parallax effects]; Kuijken et al a0707-MNRAS
[by cosmic strings].
Weak Lensing
* Idea: Gravitational
lensing that produces a small distorsion in images of background galaxies;
It cannot be recognized as lensing on the basis of a single galaxy image, but
one uses the statistical properties of many galaxies in a region of
the sky.
@ General references: Bartelmann & Schneider PRP(01);
Mellier & van
Waerbeke CQG(02)in.
@ In various gravity theories:
Acquaviva et al PRD(04)ap, ap/04-in.
@ In cosmology: Massey et al ap/04-in
[dark matter and dark energy]; Munshi et al PRP(08), Hoekstra & Jain a0805-ARNPS
[rev].
References
@ General: Ohanian AJP(87);
Blandford et al Sci(89);
in Texas XVII(95); Schechter ap/99-in
[review]; Blandford PASP(01)ap [future];
Wambsganss SA(01)nov; Perlick LRR(04)
[spacetime perspective]; Sauer a0704 [history,
Einstein and Nova Geminorum 1912]; Jain NJP(07) [focus issue].
@ Theory: Frittelli & Newman PRD(99)gq/98;
Kling et al PRD(00)gq/99 [iterative];
Frittelli et al PRD(00)gq [Schwarzschild],
PRD(01)gq/00,
PRD(01)gq/00 [image
distorsion], PRD(02)gq [non-perturbative];
Kochanek et al ap/00/ApJ
[Einstein rings]; Hasse & Perlick
GRG(02)gq/01 [and
centrifugal force reversal]; Frittelli MNRAS(03)ap [by
moving lenses]; Suyama et al PRD(05)ap [wave
propagation and thin lenses]; Amore & Arceo PRD(06),
Amore et al PRD(06)
[analytical expressions]; Werner mp/07/JMP
[topological invariants, fixed point theorem].
@ Intros, reviews: Turner SA(88)jul; Narayan & Bartelmann ap/96;
Straumann ap/97;
Schneider et al 92; Wambsganss LRR(98)ap;
Fluke et al ap/98/MNRAS
[new method]; Mollerach & Roulet
IJMPA(00)ap/99;
Wambsganss ap/00-in,
ap/06-in;
Kuijken ap/03-ln;
Koopmans & Blandford PT(04)jun
[and applications]; Falco NJP(05).
@ Of other electromagnetic waves: Lu & Pen a0710-MNRAS
[21-cm radiation, diffuse].
@ Of gravitational waves: Wang et al PRL(96);
De Paolis et al A&A(02)ap.
@ And other theories: Sereno PRD(03)ap [metric
theories]; Schimd et al PRD(05)ap/04 [scalar-tensor
including quintessence]; Keeton & Petters PRD(05),
PRD(06)
[use to test gravity theories]; Capozziello et al PRD(06)ap
[4th-order gravity]; Zhao ap/06-ln,
Chen a0712-JCAP
[TeVeS]; Ruggiero a0712 [f(R),
Palatini approach]; Schmidt a0805-PRD [f(R) gravity, DGP, TeVeS].
@ Related topics: Asada & Kasai PTP(00)ap [lens
rotation]; Frutos-Alfaro AJP(01)ap/02 [visualization
program];
Ciufolini & Ricci gq/03/PRL
[and time delay]; Nemiroff ApJ(05)ap
[magnifying gravity]; > s.a. higher-dimensional
gravity; philosophy of science; tests
of lorentz invariance.
Main page – Abbreviations – Journals – Comments – Other
sites – Acknowledgements
Send feedback and suggestions to bombelli at olemiss.edu – Modified
5 jul 2008