|  Variation of Physical Constants | 
In General > s.a. cosmology [future of the universe];
  gravitational phenomenology; modified gravity.
  * History: Predicted by
    a number of theories, such as Kaluza-Klein; 1912, Einstein worked on
    variable-c gravity; 1937, Dirac proposed that α
    could vary; 1955, Landau proposal; Bimetric theories predict a variation
    of c; 2009, Variations of constants of nature and acceleration of
    the universe could be related and governed by the evolution of a single field.
  @ Reviews, status:
    Carilli pw(01)oct;
    Chiba gq/01-proc;
    Martins PTRS(02)ap;
    Uzan ap/04-proc;
    Olive & Qian PT(04)oct;
    Barrow & Webb SA(05)jun;
    Barrow PTRS(05)ap;
    news SFN(05)dec,
    space(06)jul;
    Dent AIP(07)hp/06;
    Flambaum IJMPA(07)-a0705;
    Melnikov G&C(07);
    Fritzsch NPPS(10);
    Peik NPPS(10);
    Berengut & Flambaum JPCS(11)-a1009;
    Chiba PTP(11)-a1111;
    Calmet & Keller a1410;
    Solà MPLA(15)-a1507;
    Levshakov a1603-proc [astrophysical methods];
    Martins RPP(17)-a1709.
  @ General references:
    Belinchón & Alfonso-Faus IJMPD(01)gq/04 [\(\hbar\)c = const];
    Armendáriz-Picón PRD(02) [model];
    Langacker IJMPA(04)hp/03-conf [and extra dimensions];
    Buchalter ap/04 [c, G, h, cosmology];
    Ignatiev & Carson PLA(04) [e, \(\hbar\), c: constraints];
    MacGibbon ap/06,
    PRL(07)-a0706 [maximal rate allowed by second law of thermodynamics];
    Flambaum AIP(06)phy;
    Martins ap/06-proc [and dark energy];
    Shaw gq/07 [possible seasonal changes];
    Nea RPP(07) [comparisons of atomic frequency standards];
    Fritzsch MPLA(08);
    Uzan a0907-proc,
    LRR(11)-a1009 [general relativity extensions, cosmology];
    Dent a1005-MG12;
    Levshakov et al ApJ(11)-a1106 [use of methanol lines as tracers];
    Monteiro et al a1309-proc,
    Thompson a1602-MG14 [and fundamental physics].
  @ Theory:
    Barrow gq/97-ln;
    Dzuba et al PRL(99)phy/98;
    Vilenkin PRL(98)ht;
    Barrow & O'Toole MNRAS(01)ap/99 [in space];
    Duff ht/02;
    Uzan RMP(03)hp/02;
    Rich AJP(03)oct-phy/02 [consequences];
    Barrow ASS(03)gq/02-proc;
    Vucetich AIP(03)ap/02 [models];
    Marion et al PRL(03)phy/02,
    Fischer et al PRL(04)phy/03 [lab experiment];
    Dent et al PRD(08)-a0808;
    Flambaum PRL(09)-a0808 [critique of black-hole bounds],
    reply MacGibbon PRL(09)-a0810;
    Dent et al PRD(09)-a0812 [comparison of bounds];
    Damour SSR(09)-a0906-conf [and the equivalence principle];
    Flambaum & Berengut IJMPA(09);
    Thompson MNRAS(12)-a1202 [in slow-roll quintessence];
    Duff a1412;
    Fritzsch et al EPJC(17)-a1605 [in running vacuum models];
    Hassan et al a1807 [from non-perturbative matter-gravity theories];
    > s.a. early-universe nucleosynthesis.
  @ And other physics:
    Gleiser & Taylor PRD(85),
    PRD(86) [and Kaluza-Klein theory];
    Nunes et al a0910-proc [and cosmological acceleration];
    Kozlov & Levshakov AdP(13)-a1304 [and molecular transitions];
    Ivashchuk & Melnikov G&C(14)-a1401 [in 10D "Friedmann-Calabi-Yau" superstring cosmology];
    Thompson Univ-a1702-proc
      [constraints on particle physics parameters].
Specific Constants > s.a. electron
  [mass]; fine-structure constant; variation
  of newton's gravitational constant.
  * Variation of c:
    It can be produced in at least two different ways, a classical mechanism
    arising from the coupling of the electromagnetic field to other fields,
    and a quantum one arising from the interaction of photons with virtual
    charged-particle pairs in possibly different vacua.
  * Variation of e/p
    mass ratio: Given that gluons, not quarks, make up most of the proton's mass,
    variations in μ = mp
    / me could arise if the strong
    nuclear force changes in time, as some theorists have speculated; 2015,
    No evidence of variation over a look-back time of 11.4 Gyr.
  @ Variation of c: Dicke RMP(57) ['electromagnetic' theory of gravitation];
    Tiwari in(80)gq/02;
    Ellman phy/98;
    Moffat ap/98-fs;
    Coule MPLA(99);
    Albrecht AIP(99)ap;
    Manida gq/99;
    Clayton & Moffat PLB(99)ap/98,
    PLB(00),
    PLB(01)gq/01 [bimetric];
    Carlip PRD(03)gq/02 [and black-hole thermodynamics];
    Magueijo 03,
      RPP(03)ap;
    Ellis & Uzan AJP(05)mar-gq/03;
    Bel gq/03;
    Jafari & Shariati IJMPD(04)gq/03 [as reformulations of special relativity];
    Ellis GRG(07)ap [requirements on theories],
    comments Magueijo & Moffat GRG(08)-a0705;
    Iorio GRG(09)-a0901 [planetary tests];
    Izadi & Shojai CQG(09) [in extended-gravity theories];
    Qi et al PRD(14)-a1407;
    Coumbe a1509-MG14 [and dimensional reduction];
    Salzano et al PRD(16)-a1511 [with future galaxy surveys];
    > s.a. mach's principle; vacuum phenomenology.
  @ Variation of c and G:
    Avelino & Martins PLB(99)ap [cosmology].
  @ Variation of G and Λ: Sharif & Kausar JKPS(09)-a0911 [Bianchi III and Kantowski-Sachs cosmologies].
  @ Varying-speed-of-light cosmology:
    Barrow PRD(99);
    Magueijo PRD(09)-a0807 [bimetric, primordial fluctuations];
    Roshan et al PLB(09)-a0901 [solutions];
    Afshordi & Magueijo PRD(16)
    + news csm(16)nov [bimetric, critical geometry and scalar perturbations].
  @ e/p mass ratio: Barshay & Kreyerhoff ap/07 [and a small cosmological constant];
    Dent EPJST(08)-a0802-ln;
    Avelino PRD(08) [and α];
    Malec et al MNRAS(10)-a1001,
    in(09)-a1001 [optical molecular transitions];
    Landau & Scóccola A&A(10)-a1002 [and α];
    Landau et al APP(12)-a1010 [depending on the local value of the Weyl tensor];
    van Weerdenburg et al PRL(11)-a1104;
    Bagdonaite et al ApJ(14)-a1308,
    PRL(13);
    Mohamadnejad MPLA(19)-a1806 [from variation of Higgs VEV with cosmic time].
  @ Coupling constants: Chamoun et al PLB(01) [strong coupling constant];
    Kostelecký et al PRD(03) [and Lorentz violation];
    Shaw & Barrow PRD(05)gq/04 [electroweak, quantum corrections];
    Bambi & Drago APP(08)-a0711 [bounds from GRBs];
    Ferrero & Altschul PRD(10) [Fermi constant GF];
    Ferreira & Martins PRD(15)-a1506 [stability].
  @ QCD parameters:
    Dmitriev & Flambaum PRD(03)ap/02 [\(m^~_q/\Lambda^~_{\rm QCD}\)];
    Beane & Savage NPA(03)hp/02 [\(m^~_q\) and nuclear physics];
    Damour & Donoghue CQG(11)-a1104 [and lunar laser ranging];
    Fischbach et al a1505-proc [indications of time-varying nuclear decay constants].
  @ Planck's constant:
    Seshavatharam1 & Lakshminarayana IJA(13);
    Mangano et al IJMPA(15)-a1509 [theory];
    de Gosson & Mohageg a1612 [dependence of quantum states on h];
    de Gosson a1706
      [consequences for transitions between pure and mixed quantum states].
  @ Other constants: Bekenstein & Sagi PRD(08)-a0802 [\(G\) and Milgrom's \(a^~_0\) MOND parameter];
    Scherrer a0903 [time variation of π :-)];
    Milgrom PRD(15)-a1412 [MOND parameter].
  > Various theories:
    see brane cosmology; cosmological
    constant; dark matter;
    FLRW models; gravitation
    ["variable lightcone"]; inflationary phenomenology;
    quantum cosmology; quantum geometrodynamics;
    relativistic cosmology; renormalization;
    types of gauge theories [with varying effective charge].
Bounds and Phenomenology
  > s.a. cosmic acceleration; modified lorentz
  symmetry; scalar-tensor gravity; spacetime
  singularities.
  * c, status:
    2002, P Davies et al say examination of black holes and thermodynamics
    suggests that \(\dot\alpha/\alpha\) is due to \(\dot c\).
  * e/p mass ratio, status:
    2006, Evidence from extreme UV lines of H for a 0.002% change over 12 Gyr, at the
    3.5-σ level; 2007, Stronger upper bound of (−1 ± 3)
    × 10−16/yr [from the inversion spectrum of ammonia]; 2008,
    Upper bound (−3.8 ± 5.6) × 10−14/yr; 2009, Integrated
    Δμ/μ measured is (−7 ± 8) × 10−6;
    2011, New bound (0.3 ± 3.2stat ± 1.9sys)
    × 10−6 from z = 2 to current time; 2013, Tighter
    bounds; 2014, \(\dot\mu/\mu\) = 0.2(1.1) × 10−6/yr.
  @ General references: Sisterna & Vucetich PRD(90);
    Nordtvedt IJMPA(02)gq [and equivalence principle];
    Olive et al PRD(02);
    Chengalur & Kanekar PRL(03)ap,
    Kanekar et al PRL(05) [using OH lines];
    Rich AJP(03)oct-phy/02 [consequences];
    Shaw & Barrow PRD(06)gq/05,
    PLB(06)gq/05,
    PRD(06)gq,
    Barrow & Shaw GRG(07)gq/06 [local effects];
    Kanekar MPLA(08)-a0810 [techniques];
    Landau et al PRD(08) [fine-structure constant, Higgs vacuum expectation value, electron mass];
    Shaw & Barrow a1002-proc [constraints from seasonal variations];
    Kanekar et al ApJ(10)
    + news ns(10)jun [from conjugate radio-wave absorption and emission lines in gas cloud spectrum];
    Rellergert et al PRL(10);
    Curran et al A&A(11)-a1108;
    Kanekar et al ApJL(12)-a1201;
    Levshakov et al A&AL(12)-a1203;
    Rahmani et al MNRAS(12)-a1206 [using 21-cm absorbers];
    Leite & Martins PRD(16)-a1607 [constraints on Bekenstein-type models];
    Hart & Chluba MNRAS(18)-a1705;
    Amendola et al JCAP(18)-a1712 [Planck mass, from direct detection of gravitational waves];
    Pašteka et al PRL(19) [monitoring the size of solids].
  @ Spatial variation: Barrow PRD(05)ap [cosmological bounds];
    Levshakov et al A&A(10)-a1004 [\(\alpha^2/(m_e/m_p)\) in the Milky Way galaxy];
    Berengut et al PRD(11)-a1009;
    Iorio MNRAS(11)-a1104 [orbital effects].
  @ Dependence on gravitational potential: Dent PRL(08) [Eötvös-type bounds];
    Bagdonaite et al PRL(14)-a1409 [e/p mass ratio].
  @ And nucleosynthesis:
    Ichikawa & Kawasaki PRD(02);
    MacDonald & Mullan PRD(09)-a0904 [strong force and anthropic principle];
    Coc et al a1301-proc.
  @ And inflation: Martins ap/00-conf;
    Chamoun et al IJMPD(07)ap/06 [strong coupling constant].
  @ Planck's constant: Kentosh & Mohageg PRL(12)-a1203,
    comment Berengut & Flambaum PRL(12)-a1203 [from GPS clock-correction data];
    Calmet PTRS(15)-a1504 [energy scale dependence, bounds];
    Huang PRD(16)-a1511 [observational effects].
  @ e/p mass ratio:
    Tzanavaris et al PRL(05)ap/04,
    MNRAS(07)ap/06 [21-cm + UV lines];
    Barrow & Magueijo PRD(05)ap [cosmological constraints];
    Ivanchik A&A(05)ap;
    Reinhold et al PRL(06)
    + pn(06)apr [evidence];
    Chiba et al PRD(07);
    Flambaum & Kozlov PRL(07)
    + pw(07)jun;
    Shelkovnikov et al PRL(08) [lab constraint];
    Murphy et al Sci(08)jun
    + sr(08)jun,
    King et al PRL(08)-a0807 [quasar spectra];
    Thompson et al ApJ(09)-a0907 [consistent with no change over 11.5 Gyr];
    Levshakov et al IAU-a0911;
    Beloy et al PRA(10) [diatomic molecules];
    King PhD(11)-a1202 [quasar absorption lines];
    King et al MNRAS(11)-a1106 [H2 transitions in quasar spectra];
    Bagdonaite et al Sci(12)dec
    + news at(12)dec [ethanol torsional spectrum];
    Levshakov et al a1307-proc;
    Wendt AN(14)-a1310 [based on H2 observations];
    Huntemann et al PRL(14),
    Godun et al PRL(14) [atomic clock measurements];
    Kanekar et al MNRAS(15)-a1412 [methanol lines];
    Bagdonaite et al PRL(15);
    Daprà et al MNRAS(15)-a1509 [from H2 absorption];
    Owens et al MNRAS(15) [from vibrations of hydronium, protonated water];
    Ubachs et al RMP(16)-a1511 [with H2 quasar absorption method];
    Ubachs SSR(18)-a1709-conf.
  @ Variation of c: Albrecht & Magueijo PRD(99) [cosmology];
    Bekenstein ap/03 [and lab spectroscopy].
  >  Related topics:
    see torsion and physical theories
    [constraints on f(T) gravity].
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