|  Modified Newtonian Dynamics (MOND) | 
In General > s.a. variation of constants.
  * Idea: At accelerations below
    a certain value a0 (g
    = ∇Φ < a0),
    Newton's second law of dynamics is replaced by F
    = ma2/a0.
  * History: 1983, Proposed by
    Milgrom as a way to explain flat galactic rotation curves without the need
    for dark matter; To explain the flatness of the curves, one can set
    a0 ~ 1.2 × 10−10
    m/s2 ~ cH0/6;
    The effective gravitational attraction approaches (gN
    a0)1/2,
    where gN is the usual Newtonian
    acceleration; The effective force goes like 1/r at large distances.
  * Consequences: When a
    = (gN
    a0)1/2
    ("deep MOND"), a body gravitationally bound to a mass M
    will orbit with speed v4
    = a0GM, independent of distance!
    (The exponent agrees with the Tully-Fisher relation); If used as alternative to
    dark matter (but possibly with a cosmological constant), the theory predicts
    the ratio between the heights of the peaks of the cmb power spectrum; 2004,
    A1 / A2
    agrees with WMAP data, A2
    / A3 has not been reliably measured yet.
  * Status: 2004, It is a
    phenomenological proposal, possibly related to a modification of Newton's law of
    motion F = ma or of the Poisson equation for gravity, but is still
    lacking a theoretical interpretation and covariant formulation; 2004, Proposal of
    TeVeS by Bekenstein; 2007, University of Washington measurements support the validity
    of Newton's second law down to 5 × 10−14
    m/s2; 2018, More lack of evidence of a fundamental
    acceleration in galaxies.
  @ Reviews: Milgrom APPB(01)ap-ln,
    a0801-conf;
    Sanders MPLA(03);
    Scarpa AIP(06)ap;
    Frank disc(06)aug [I];
    Bekenstein CP(06)ap/07;
    Milgrom a0908 [semi-popular],
    AIP(10)-a0912;
    Dodelson IJMPD(11)-a1112-GRF,
    comment Moffat & Toth a1112 [challenges];
    Famaey & McGaugh LRR(12)-a1112;
    Famaey & McGaugh a1310-conf [phenomenology];
    Sanders CJP(14)-a1404 [historical perspective];
    Milgrom CJP(15)-a1404;
    Bugg CJP(14)-a1405 [critical appraisal];
    Sanders 16 [and concordance cosmology];
    Merritt 20 [philosophical].
  @ General papers: Milgrom ApJ(83),
    ApJ(83);
    Milgrom PLA(99)ap/98 [as vacuum effect],
    NAR(02)ap [rev];
    Sanders ap/01-conf;
    Soussa & Woodard CQG(03)ap,
    Soussa ht/03-proc [non-local formulation];
    Darabi IJTP(10)-a0908 [Machian interpretation];
    Milgrom MNRAS(10)-a0911 [quasi-linear formulation];
    Bugg CJP(13)-a1304 [novel interpretation];
    Milgrom PRD(15)-a1507 [new perspective],
    SHPMP(20)-a1910-conf [vs dark matter].
  @ Relativistic: Demir & Karahan EPJC(14)-a1408;
    Barrientos & Mendoza EPJP(16)-a1602;
    Sussman & Hernández a1908 [and cosmic expansion rate].
  @ From modified inertia: Milgrom EAS(06)ap/05-proc [modified inertia vs modified gravity];
    Wang a1011;
    Milgrom APPB(11)-a1111-conf;
    Namouni MNRAS-a1504;
    Costa et al a1904 [local Lagrangian].
  @ As weak-field limit of extended metric theories: 
    Bernal et al EPJC(11)-a1108,
    Mendoza et al AIP(12)-a1202;
    Barrientos & Mendoza PRD(18)-a1808.
  @ Other origin: Jordan ap/04 [acceleration fluctuations];
    Kao ap/06 [extra dimension];
    Blanchet CQG(07)ap/06 [gravitational polarization];
    Zaveri PiP-a0805;
    Zhao a0805 [neutrino-gravity coupling];
    Milgrom ApJ(09)-a0810 [and spacetime scale invariance];
    Pikhitsa a1010 [from gravitational thermodynamics];
    Sebastian & Kuriakose a1104 [boundary terms in the gravitational Hamiltonian];
    Bernal et al MPLA(11)-a1110 [acceleration scale as fundamental quantity];
    Trippe JKAS(13)-a1303 [from massive gravitons];
    Carranza & Mendoza JModP(15)-a1402 [as an entropic force];
    Schiffer a1403 [cosmological expansion?];
    Milgrom a1804-in [from a brane-world picture];
    Giusti a2002,
    Varieschi a2003 [based on fractional calculus formalism];
    > s.a. entropic gravity.
  @ Other applications:
    McLaughlin & Meylan ap/03-in [MOND not needed];
    Ciotti & Binney MNRAS(04)ap [two-body relaxation].
  @ Other consequences: Ignatiev PRL(07)gq/06
    + news pw(07)mar [possible violation of Newton's second law – SHLEM];
    Shariati & Jafari a0710 [and conservation of energy];
    Ignatiev PRD(08)-a0802 [test using high-latitude effect on Earth];
    > s.a. black holes.
  @ Alternatives: Romero & Zamora PRD(06)ap;
    Blanchet et Combes Rech-a0910 [dipolar matter];
    Rastall CJP(14)-a1401 [theory with two separate forces].
  > Online resources:
    see the MOND Pages;
    Wikipedia page.
And Gravitation
  > s.a. MOND and astrophysics / cosmology; jacobi dynamics;
  Mimetic Gravity; MOG; TeVeS;
  theories of gravitation.
  * AQUAL: An implementation
    of MOND as a non-relativistic modified-gravity theory.
  * External field effect: In MOND,
    the internal dynamics of a gravitating system s embedded in a larger one
    S is affected by the external background field of S even if it is
    constant and uniform, thus implying a violation of the Strong Equivalence Principle.
  @ General references: Mendes & Opher PLB(01)ap [sub-mm tests];
    Roscoe GRG(04);
    Bekenstein PRD(04)ap;
    Sanders LNP(07)ap/06;
    Bruneton & Esposito-Farèse PRD(07)-a0705;
    Bekenstein NPA(09)-a0901 [rev, AQUAL],
    in(10)-a1001 [rev];
    Zhao et al PRD(10)-a1007;
    Skordis & Zlosnik PRD(12)-a1101 [geometry];
    Fazy PRD(13)-a1302 [MOND as quantum-statistical modified entropic gravity];
    Smolin PRD(17)-a1704 [as a regime of quantum gravity].
  @ Bimetric MOND gravity: Milgrom PRD(09)-a0912;
    Milgrom MNRAS(10)-a1001 [and twin matter];
    Clifton & Zlosnik PRD(10)-a1002 [FLRW cosmology];
    Milgrom PRD(10)-a1006 [growth of perturbations];
    Milgrom PRD(14)-a1308 [gravitational waves];
      Milgrom a1310-conf [rev].
  @ Other theories: Kao gq/05 [and induced gravity];
    Zlosnik et al PRD(06)gq [vector-tensor theory];
    Falcon a1007 [and FLRW cosmology];
    Woodard CJP(14)-a1403
      [MOND as non-local residual effect from the vacuum polarization of infrared gravitons];
    Barrientos & Mendoza EPJP(17)-a1612 [as the weak-field limit of a theory with torsion];
    Christodoulou & Kazanas a1901 [as low-acceleration limit of G(a) gravity];
    Skordis & Złosnik a2007;
    Barrientos et al a2008 [with curvature-matter couplings];
    > s.a. hořava gravity.
  @ Solutions, special systems: Giannios PRD(05) [spherical static solutions];
    Malekjani et al ApJ(09)-a0811 [spherical collapse].
  @ Proposed tests: Gundlach et al PRL(07)
    + pw(07)apr [lab test];
    De Lorenci et al A&A(09)-a1002 [small-acceleration test];
    Trenkel et al a1001 [LISA];
    Magueijo & Mozaffari PRD(12)-a1107 [LISA Pathfinder];
    Das & Patitsas PRD(13)-a1305 [in freely-falling laboratories];
    > s.a. equivalence principle.
  @ Other phenomenology:
    Zhao & Famaey PRD(10) [virial theorem and elliptical shells];
    Milgrom PRL(11) [and gravitational Cerenkov losses];
    Milgrom MNRAS(12)-a1205 [in isolated high-acceleration systems];
    Golovnev & Masalaeva GRG(14)-a1306 [gravitational collapse];
    Milgrom PRD(14)-a1311 [virial theorem in general theories];
    Blanchet & Bernard IJMPcs(14)-a1403 [and gravitational polarization];
    Chesler & Loeb PRL(17)-a1704
      [fatal inconsistencies of two relativistic generalizations with gravitational-wave observations];
    Klein CQG(20)-a1901 [evidence from Cavendish-type experiments].
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