|  Gamma-Ray Bursts | 
In General
  > s.a. gamma-ray astronomy / sources
  of gravitational waves; cosmological parameters.
  * 1998: Are they due to the
    coalescence of binary neutron stars? A typical length is about 100 s.
  * 1999: First one observed
    optically while active; They seem to signal the birth of stellar-mass
    black holes.
  * 2006: They only tend
    to occur in small, misshapen "metal-poor" galaxies, unlike the Milky Way
    [@ news pw(06)apr].
  * 2009: GRB 090423,
    seen by the Swift satellite, had z = 8.3 [@ news
    NASA(09)apr;
    Tanvir et al Nat(09)-a0906;
    news ns(09)oct].
  * 2012: Their
    status as sources of high-energy cosmic rays questioned by IceCube results
    showing too few neutrinos coming from GRBs.
  * 2013: Evidence
    that short-duration grbs (lasting less than two seconds) are produced by
    the merger of compact objects, such as neutron stars. 
  * 2016: There is
    mounting evidence for the binary nature of the progenitors.
  @ General references: Piran GRG(96)gq,
    PRP(99)ap/98,
    PRP(00)ap/99-proc [fireball model];
    Tavani ap/98-conf;
    Heinz & Begelman ApJL(99)ap [shotgun model];
    Woosley AIP(00)ap/99 [engine];
    Zimmerman ThSc(00)jan; Zhang Nat(06)ap [new type];
    Lamb NCB(06) [and cosmology];
    Lü et al ApJ(10)-a1001 [classification];
    news at(12)apr [IceCube detector sees too few neutrinos for fireball model];
    Littlejohns et al MNRAS(13)-a1309 [high vs low-redshift];
    Ruffini et al ApJ(16)-a1602 [sources];
    Zhang 18 [physics].
  @ Reviews: Hartmann ThSc(92)jul [sources];
    Fishman & Hartmann SA(97)jul;
    Rees ap/97;
    Mészáros PTPS(99)ap-conf;
    Piran gq/02-GR16,
    RMP(04)ap;
    Hjorth et al pw(04)oct;
    Mörtsell & Sollerman JCAP(05)ap [future];
    Mészáros RPP(06)ap;
    Ghisellini PoS-ap/06 [and blazars];
    De Rújula a0711-ln;
    Grindlay Nat(08)sep-a0901 [long-lasting];
    Stamatikos IJMPD(09)-a0904-proc;
    Vedrenne & Atteia 09;
    McBreen et al a1003-proc;
    Nakar a1009-proc;
    Ghisellini IAU(11)-a1010;
    Ruffini IJMPD(11)-a1107-MG12,
    Rico a1111-proc [and fundamental physics];
    Mészáros APP(12)-1204;
    Gomboc CP(12)-a1206;
    Berger ARAA(14)-a1311 [short-duration GRBs];
    Kumar & Zhang PRP(15)-a1410;
    Horváth a1903 [hist];
    Rueda et al Univ-a1905.
  @ And cosmology: Bromm & Loeb a0706-in [as early-universe probes];
    Amati a0908-proc [cosmological parameters];
    Tsutsui et al a1205/JCAP [as distance indicators];
    Wei & Wu IJMPD(17)-a1607-MG14 [as standard candles].
  @ Spectral time lags: Pavlopoulos PLB(05)ap; Amelino-Camelia et al a1707;
    Chaichian et al a2101-conf [explanations without Lorentz symmetry breaking].
  @ Other effects: Annis JBIS(99)ap [and life];
    Thomas et al ApJ(05)ap [on Earth];
    Kocevski & Petrosian a1110/ApJ [time-dilation effects];
    news bbc(13)jan [AD 774-775];
    Piran & Jimenez PRL(14) [life extinctions];
    Gowanlock ApJ(16)-a1609 [astrobiological].
  @ Related topics: King et al ApJL(05)ap [restarting the engine];
    Savaglio NJP(06) [as probes of chemical evolution];
    Lieu ApJ(08)ap/07 [gravitational time delay];
    Bloom et al ApJ(09)-a0803 [naked-eye GRB 080319B];
    Song a0805 ["redshift is gravitational"];
    Dado & Dar a0910/ApJ [high-energy photons];
    news nat(10)nov [and magnetars];
    Coward et al PoS-a1206 [optical selection effects];
    Shenoy et al ApJ(13)-a1304 [curvature effects];
    Wiersema et al Nat(14)may [circular polarization in the optical afterglow];
    > s.a. neutrinos;
      neutron stars [GRB precursors].
  > And quantum gravity: see quantum
    gravity phenomenology; tests of lorentz violation.
Sources and Mechanisms
  * Types: Long "soft"
    ones (with a duration > 2 s) are due to massive star collapse explosions;
    Short, hard ones (0.1 s or so) to compact binary coalescence.
  * Models: Fireball (synchrotron
    radiation from colliding shells); Cannonball (jet from infalling matter).
  @ Theory: Mészáros ARAA(02)ap/01;
    Dermer ap/02-conf;
    De Rújula ap/03-proc;
    Dar & De Rújula PRP(04)ap/03;
    Amelino-Camelia hp/05-conf [and Planck-scale physics];
    Covino Sci(07)-a0705 [mechanism];
    Lyutikov a0911-proc;
    Granot & Ramírez-Ruiz a1012-ch [and jets];
    Piran et al a1206-proc [origin];
    Rezzolla & Kumar ApJ(15)-a1410 [short GRBs, novel paradigm].
  @ Supernovas: Mohapatra et al APP(00)ap/99 [mirror supernovas];
    Paczyński ap/99-proc;
    Soderberg AIP(06)ap [rev];
    Woosley & Bloom ARAA(06);
    Hjorth & Bloom a1104-ch;
    Cano a1208-PhD.
  @ Microscopic / primordial black holes: Casadio et al AIP(02)ap;
    Cline & Otwinowski a0908 [estimate].
  @ Superconducting cosmic strings: Berezinsky et al PRD(01)ap/00;
    Cheng et al PRL(10)-a1005
    + news ng(10)aug.
  @ Neutron stars: Rosswog ap/05 [neutron star–black hole binaries];
    Ruiz et al ApJ(16)-a1604 [binary neutron star mergers].
  @ Simulations on Earth:
    Warwick et al PRL(18)
    + news giz(18)jan [plasma beam].
  @ Sources, other: Kundt ChJAA-ap/03 [galactic origin?];
    Paczyński & Haensel MNRAS(05)ap [and quark star formation – support
      in Lazzati MNRAS(05)ap/04];
    Virgili et al ApJ(11)-a0909;
    Metzger et al MNRAS(11)-a1012 [proto-magnetar model].
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