|  Cosmic-Ray Sources | 
In General
  * Primary source:
    1990, Not yet exactly known; Probably multiple origin, with lower-energy
    (< 1015 eV) electrons and ions accelerated
    by supernova shocks in our galaxy, and more energetic ones extragalactic;
    1995, First evidence of cosmic rays from supernova [@ Koyama et al
    Nat(95)nov];
    2007, High-energy cosmic rays originate in AGNs (probably accelerated by a
    stochastic process of multiple bounces off moving clouds carrying magnetic
    fields); 2009, Gamma-ray emission from ordinary galaxies supports idea that
    lower-energy cosmic rays originate mostly from shock waves in supernova
    remnants, although some argue that the link is actually to star-forming regions
    rather than SNRs; 2013, Supernova origin of galactic cosmic rays confirmed.
  @ General references: Dar & De Rújula PRP(08)hp/06 [single type of extrasolar source];
    Abraham et PA a0907-conf;
    Drury APP(12)-a1203;
    Istomin a1406 [extragalactic and galactic];
    Drury a1412-conf.
  @ Galactic center: Guo et al NJP(13)-a1101-ln;
    Istomin NA(14)-a1110;
    Abramowski et HESS Nat(16)mar-a1603 [PeV protons];
    Fujita et al a1603 [Sgr A*].
  @ Other galactic sources: Butt Nat(09)aug-a1009;
    Prantzos A&A(12)-a1112;
    Blasi NPPS(13)-a1211;
    news pw(13)feb;
    Amato IJMPA(14).
  @ Extragalactic sources:
    Kashiyama & Mészáros ApJL(14)-a1405 [galaxy mergers];
    Settimo a1612-proc [rev].
  @ Supernovae: Dar NCB(04)ap/04 [bipolar jets];
    Berezhko & Voelk ApJL(07)-a0704 [remnants];
    Tatischeff PoS-a0804;
    Cardillo et al NPPS(14)-a1410;
    Morlino a1611-ch,
    a1706-IAU [rev].
  @ Galactic vs extragalactic: Allard et al APP(07)ap/05;
    Aloisio et al PRD(08);
    Berezinsky APP(14)-a1301-conf [signatures].
  @ Other types of sources: Vachaspati PRD(10) [from cusps on cosmic strings].
  @ Anisotropy: Mollerach a0902-proc;
    Toscano et IceCube a1011,
    news livesci(10)aug [evidence from IceCube];
    Giacinti et al JCAP(12)-a1112 [and transition from galactic to  extragalactic cosmic rays];
    Deligny a1612-eConf [rev].
 Other aspects: see cosmic rays; UHE
  cosmic rays; propagation [including acceleration mechanisms].
  Other aspects: see cosmic rays; UHE
  cosmic rays; propagation [including acceleration mechanisms].
Spectrum
  * Spectrum: The observed energy
  spectrum of cosmic rays on earth is not the source spectrum of these particles.
  @ Sources, spectra:
    Abdo et FLAT PRL(09)
    + Winstein & Zurek Phy(09)
      [e+-e− spectrum, 20 Gev–1 keV];
    Abraham et PA a0907-conf [spectrum];
    Schwarzschild PT(10)jan;
    Halzen a1010-conf;
    PA Collaboration a1107-conf;
    > s.a. high-energy cosmic rays [acceleration].
  @ Spectrum, Tsallis statistics: Beck PhyA(04);
    Włodarczyk & Wilk a0706-conf [thermal sources].
  @ Spectrum features:
    Apel et KASKADE-Grande Collaboration PRL(11) [second knee-like structure];
    Giacinti et al PRD(14)-a1403 [the knee and cosmic-ray escape from the galaxy];
    Deligny CRP(14)-a1403 [interpretation of the ankle];
    Giacinti et al PRD(14) [spectrum above the knee as escape from the galaxy];
    Widom et al a1501
      [the knee as sign of a second-order phase transition].
Ultra-High-Energy Cosmic Rays > s.a. GZK Effect.
  * Idea: The most likely candidates
    are supernovae, gamma-ray bursts (GRBs) and active galactic nuclei (AGNs).
  @ General references: Farrar ap/05 [5-event cluster];
    Pierpaoli & Farrar ap/05 [galaxy clusters];
    Jain & Panda ap/05 [not primordial black holes];
    Erlykin & Wolfendale JPG(05)ap;
    Blasi MPLA(05)ap;
    Inoue ap/07-conf;
    Fraschetti PTRS(08)-a0809 [rev, and propagation];
    Waxman & Loeb JCAP(09)-a0809 [transient sources];
    Katz et al JCAP(09) [flux and spectrum];
    Farrar et al a0904,
    a0904 [correlations];
    Albuquerque & Chou JCAP(10)-a1001 [highest-energy Auger event];
    Aloisio & Boncioli APP(11)-a1002 [model for effects of source distribution];
    Piran a1005 [composition and distances];
    Stanev MPLA(10) [review];
    Dado et al NCC-a1011;
    Vladimirov et al ApJ(12)-a1108;
    Pe'er & Loeb JCAP(12)-a1111 [constraints from high-energy Fermi satellite observations]; 
    Yoshida & Ishihara PRD(12) [and neutrinos];
    Aloisio EPJwc(13)-a1207 [galactic and extra-galactic];
    Blasi CRP(14)-a1403;
    Anchordoqui a1707-proc;
    Fargion PoS-a1805.
  @ AGNs: Auger Collaboration Sci(07)-a0711
    + pw(07)nov
    + PT(08)jan [nearby];
    Gorbunov et al a0804;
    Moskalenko et al ApJ(09)-a0805,
    Stanev a0805 [criticism];
    Nagar & Matulich A&A(08)-a0806 [Auger, nearby radio galaxies];
    Hardcastle et al MNRAS(09)-a0808 [Centaurus A];
    Biermann et al IJMPD(09);
    Fraija et al a1007 [Cen A];
    Nemmen et al ApJ(10)-a1007 [Fermi data];
    Kim & Kim JCAP(11)-a1009,
    IJMPD(13)-a1203 [statistical analysis].
  @ GRBs: 
    news pw(12)apr [surprisingy few neutrinos from GRBs seen by IceCube];
    news ns(12)jul [possible after all];
    Mészáros NPPS(14)-a1407 [rev].
  > Online resources:
    see NASA 2017 video.
 main page
  – abbreviations
  – journals – comments
  – other sites – acknowledgements
  send feedback and suggestions to bombelli at olemiss.edu – modified 8 oct 2018