|  Dark Matter | 
In General > s.a. observational
  cosmology; types of dark matter.
  * Idea: Matter that interacts only gravitationally
    and possibly through the weak force and is thus very hard to detect, but can account for some observed
    properties of the universe; In inflation, it is necessary in order to reconcile the initial density
    fluctuations with present short-range correlations between galaxies; There may be more than one
    kind, acting on different scales.
  * Motivation:
    Galaxy rotation curves, galaxy-cluster velocity dispersions, gravitational lensing, patterns in
    large-scale structure (clustering, filaments, voids) , separation between mass and ordinary matter
    in colliding galaxy clusters, galaxy correlation functions, cmb anisotropies.
  * Status: 2018, The existence of dark matter is accepted
    by the vast majority of astrophysicists, but there is a minority who think it doesn't exist and
    that the effects attributed to it are a consequence of modified gravity.
  * Outstanding issues: Quantitatively reproduce the
    internal motions of galaxies and the Tully-Fisher relation; 2018, Explain the fact that satellite
    galaxies orbiting larger galaxies tend to be distributed on a single plane, at least in the case
    of the Milky Way, M31 and Centaurus A.
Effects, Indirect Evidence
  > s.a. cosmic rays; dark-matter detection;
  dark-matter distribution; gamma rays.
  * Dynamical methods:
    Transverse motion of stars in our galaxy; Differential rotation of
    our galaxy and other spirals; Escape velocity from our galaxy (lower
    bound from highest star velocities seen); Internal motions in
    galaxy clusters, including Milky Way satellites in the Local Group;
    These are sensitive to clustering below the probed scale.
  * Other methods:
    Flatness of the universe and observed density.
  * Astrophysical effects:
    If ultralight bosons exist in nature, they would cause superradiant
    instabilities in spinning black holes ("black-hole bomb"),
    although the timescale for the instability is typically very large
    (> s.a. matter around black holes).
  @ Reviews: Roncadelli ap/03-proc;
    Mambrini & Muñoz JCAP(04)hp [vs direct];
    De Freitas & Peirani G&C(05)ap [searches];
    Bertone & Merritt MPLA(05)ap;
    Mavromatos a1111-conf [theoretical scenarios];
    Roos JModP(12)-a1208,
    Luković et al IJMPA(14) [in astrophysics and cosmology];
    Cirelli a1511;
    Gaskins CP(16)-a1603 [indirect searches].
  @ Galactic rotation curves: Carmeli IJTP(98)ap/96 [vs expansion];
    Edery PRL(99)gq;
    Bekenstein et al PRL(00)ap/99;
    Lake PRL(04);
    Menzies & Mathews gq/06/CQG [general relativity not enough];
    Rubin PT(06)dec [M31];
    news Forbes(17)jun;
    > s.a. dark matter on cosmological scales;
      types of dark matter.
  @ Interactions:
    Ullio et al PRD(02) [into γ-rays];
    Böhm et al ap/02-conf [strength];
    Sancisi ASP-ap/03 [coupling to visible matter];
    Mangano et al PRD(06)ap,
    Serra et al PRD(10) [neutrino interactions];
    Bovy & Farrar PRL(09)-a0807 [and fifth force, bounds];
    Grib & Pavlov G&C(09)-a0810 [conversion into visible matter in AGNs];
    Palomares-Ruiz & Siegal-Gaskins JCAP(10)-a1003 [annihilations and decays];
    Stiele et al PRD(10) [self-interaction, and cosmology];
    Davoudiasl et al PRL(10)
    + news pw(10)nov [with X particles of hidden sector];
    Zheng et al NPB(12)-a1012 [constraints on interactions];
    Kouvaris PRL(12)-a1111 [self-interactions, constraints];
    Conrad a1411-in [WIMP indirect detection, rev];
    Khlopov MPLA(14)-a1411 [rev];
    news SA(15)apr [potential detection of non-gravitational self-interactions].
  @ Structure formation: Del Popolo ap/02;
    Diemand et al Nat(05)ap [small halos in the early universe];
    Silk LNP(07)ap/06;
    Primack NJP(09)-a0909 [small-scale issues];
    Boyarsky et al a0911 [matter distribution and scaling];
    > s.a. early universe; galaxy formation.
  @ And cmb: Padmanabhan & Finkbeiner PRD(05)ap [annihiliations and polarization];
    Hooper et al PRD(07)-a0705 [annihilations and WMAP haze];
    Mertsch PhD(10)-a1012 [anomalies in cosmic-ray and microwave sky maps].
  @ Other astrophysics and cosmology:
    Blanchard & Douspis A&A(05)ap/04 [clusters];
    Ahluwalia-Khalilova ap/06 [globular clusters and age of the universe];
    Iorio JCAP(06)gq [solar system orbits];
    Loeb & Weiner PRL(11) [and dwarf-galaxy cores];
    Cheung et al JCAP(14)-a1408 [in a bouncing universe];
    Loeb & Muñoz Phy(18) [21-cm absorption in light from the first stars];
    Nielsen et al a1903 [gravitational atoms].
  > Online resources:
    see fine-structure constant [variation];
    higher-dimensional gravity; perturbations.
General References > s.a. history of astronomy;
  relativistic cosmology / Conformal Gravity.
  @ Status, reviews:
    news Sci(91)jan;
    Griest ap/95-proc;
    Raffelt ap/95-proc;
    Bahcall ap/96;
    Jetzer ap/96;
    Hu et al PRD(99)ap/98;
    Bosma CMDA(98)ap-in;
    Ellis PS(00)ap/98-conf [particle candidates];
    Turner PS(00)ap/99-proc,
    ap/99-proc;
    Bergström RPP(00)hp;
    Sellwood & Kosowsky ap/00-in [Λ+CDM vs modified general relativity];
    Evans ap/01-conf [vs non-standard gravity];
    Carr ap/01-conf [MACHOS];
    Khalil & Muñoz CP(02);
    Spooner & Kudryavtsev ed-01;
    Primack ap/01-proc,
    ap/03-IAU;
    Olive ap/03-ln;
    Bergström hp/03-proc;
    Rees PTRS(03)ap/04;
    Bahcall et al ed-04;
    Muñoz IJMPA(04) [experimental];
    Sahni LNP-ap/04 [and dark energy];
    Overduin & Wesson PRP(04)ap;
    Bertone et al PRP(05) [particles];
    Frampton ap/05-conf [and dark energy, intro];
    news BBC(06)feb;
    Zacek a0707-proc;
    Peskin JPSJ(07)-a0707-ln;
    Ellis a0811-conf;
    Einasto a0901-in;
    Primack a0902-proc
      [issues with observations and simulations of galaxies];
    D'Amico et al a0907-ln;
    issue NPPS(09)194 [proc];
    Colafrancesco AIP(10)-a1004;
    Garrett & Dūda AiA(11)-a1006;
    Regis a1008-conf [particle dark matter];
    Gelmini a1009-conf;
    Matarrese et al ed-11;
    Einasto a1109-conf;
    Capozziello et al a1110-in [and alternatives];
    news sn(13)jan,
    PhysOrg(13)feb [status and predictions];
    Capozziello & Lambiase NAP-a1304;
    Peebles a1305;
    Einasto BJP(13)-a1308-TX;
    Luković et al IJMPA(14)-a1411 [in cosmology];
    Lisanti a1603-ln;
    Kunz et al PRD(16)-a1604 [and large-scale structure];
    Fornengo a1701-eConf;
    Freese a1701-MG14.
  @ I: Disney 84;
    Tucker & Tucker 88; PW(95)jun, p39;
    Krauss 89, 00;
    Hooper 06 [and dark energy];
    Freese 14;
    Blanchet & Famaey Rech-a1602.
  @ I, articles: news
      forbes(18)mar [dark matter, not modified gravity].
  @ II, articles: Krauss SA(86)dec;
    Trimble CP(88);
    Tremaine PT(92)feb;
    Auteri ap/07-proc;
    Roos a1001 [evidence];
    Lincoln TPT(13)mar [short intro].
  @ II, books: Parker 89;
    Srednicki ed-90;
    Riordan & Schramm 91;
    Sciama 93;
    Overduin & Wesson 02.
  @ And other matter:
    Mazzei ap/04 [rev];
    Wilczek hp/04-ch [anthropic reasoning];
    Bousso & Hall PRD(13) [multiverse argument].
  @ Arguments against: Milgrom SA(02)aug;
    Roberts EJTP-ap/05;
    Barak & Leibowitz a0909 [no need for dark matter or dark energy];
    Mannheim a1903-GRF.
  @ Related topics: Cline ap/05-conf [vs MOND];
    Ahluwalia IJMPD(09)-a0904 [relativity in the dark sector, Elko example];
    Capistrano & Cabral AP(14) [geometrical aspects];
    Lee a1510 [quantum entanglement];
    > s.a. anthropic principle; philosophy of physics.
  > Online resources:
    see Astronomy Today article.
Alternatives to Dark Matter
  > s.a. galaxies [no need for dark matter].
  * MOND: Modified Newtonian Dynamics
    was considered as a possible alternative for a few years; In 2002–2003 new
    data, especially from the SDSS, contradicted MOND predictions; However, some
    people are still impressed with its rotation curve predictions.
  * Other theories: Other alternatives
    include Moffat's bimetric gravity and Mannheim's conformal gravity.
  @ General references:
    Vishwakarma S&S(06)ap/04 [galaxy rotation];
    Cooperstock & Tieu ap/05/ApJ [general relativity does the job],
    commemt Garfinkle CQG(06)gq/05;
    Mégier a1409
      [non-relativistic limit of Einstein's equation in an expanding universe];
    Lopez-Corredoira a1808 [rev].
  @ MOND:
    Sanders & McGaugh ARAA(02)ap;
    Aguirre IAU-ap/03 [rev];
    Pointecouteau ap/06 [vs dark matter];
    Bekenstein in(10)-a1001.
  @ Modified gravity:
    Sellwood & Kosowsky ap/01-in;
    Mannheim PPNP(06)ap/05 [general discussion];
    Sobouti A&A(07)ap/06 [f(R) gravity];
    Chalmers pw(06)jun;
    Sereno & Jetzer MNRAS(06)ap [and solar planets];
    Vanderburgh PhSc(05)dec [conceptual];
    Kahya & Woodard PLB(07)-a0705 [proposed test];
    Brownstein & Moffat MNRAS(07)
    + pw(07)nov [Bullet cluster];
    Brownstein PhD(09)-a0908 [comparing MoG, MOND and CDM];
    Moffat a1101-conf [rev];
    Foreman & Scott PRL(12)-a1108,
    reply McGaugh a1109
      [unreliability of the baryonic Tully-Fisher relation as a test];
    Khoury PRD(15)-a1409 [dark-matter fluid + modified gravity];
    Cembranos JPCS(16)-a1512;
    Cadoni et al PLB(18)-a1707 [as an effective fluid];
    Zloshchastiev Univ-a2011 [scale-dependent gravity];
    > s.a. bimetric theories; higher-order gravity;
      theories of gravitation; unified theories [Weyl-Dirac].
  @ Related topics:
    Funkhouser gq/03 [Mach-type forces];
    Pal et al PLB(05) [effective 4D theory from branes];
    Moffat ap/06 [lensing];
    Carati & Galgani a0707-wd [outer mass distribution in (clusters of) galaxies];
    Cooperstock & Tieu MPLA(08)-a0712 [general relativistic velocity];
    Rodrigues et al JCAP(10)-a0911 [renormalization-group corrections to G];
    Barak & Leibowitz a1003;
    Hajdukovic ASS(11)-a1106
    + news PhysOrg(11)aug,
    ASS(13)
    + news ns(13)jan [gravitational vacuum polarization, and proposed test with Eris and Dysnomia];
    Bertolami et al PRD(12)-a1111 [non-minimal matter coupling];
    Koch & Wright JMOGC(12)-a1208 [turbulent flow of spacetime];
    Sanejouand a1401 [alternative form for Hubble's law];
    de Oliveira et al GRG(15)-a1501 [and Milky Way dynamics];
    Tuveri & Cadoni a1904 [quantum gravity effects];
    Deur et al a1909 [non-linear effects in general relativity].
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