Neutrinos from cosmic ray interactions in the Sun

Cosmic rays hitting the solar atmosphere generate neutrinos that interact and oscillate in the Sun and oscillate on the way to Earth. These neutrinos could potentially be detected with neutrino tel ...

[1]  J. G. Gonzalez,et al.  Search for annihilating dark matter in the Sun with 3 years of IceCube data , 2016, 1612.05949.

[2]  S. Moch,et al.  Lepton fluxes from atmospheric charm revisited , 2015, 1507.01570.

[3]  A. Mirizzi,et al.  Oscillations of solar atmosphere neutrinos , 2006, hep-ph/0608321.

[4]  P. O. Hulth,et al.  First year performance of the IceCube neutrino telescope , 2006 .

[5]  P. O. Hulth,et al.  Improved limits on dark matter annihilation in the Sun with the 79-string IceCube detector and implications for supersymmetry , 2016, 1601.00653.

[6]  S. M. Chitre,et al.  The Current State of Solar Modeling , 1996, Science.

[7]  Thomas K. Gaisser,et al.  Spectrum of cosmic-ray nucleons, kaon production, and the atmospheric muon charge ratio , 2011, 1111.6675.

[8]  T. Gaisser,et al.  A new version of the event generator Sibyll , 2015, 1510.00568.

[9]  J. Edsjö,et al.  Neutrinos from WIMP annihilations obtained using a full three-flavor Monte Carlo approach , 2007, 0709.3898.

[10]  Patrick T. Wallace.  SLALIB: A Positional Astronomy Library , 2014 .

[11]  S. Mrenna,et al.  Pythia 6.3 physics and manual , 2003, hep-ph/0308153.

[12]  Robert F. Stein,et al.  Simulations of Solar Granulation. I. General Properties , 1998 .

[13]  D. Mackay,et al.  The Sun’s Global Photospheric and Coronal Magnetic Fields: Observations and Models , 1999, 1211.6545.

[14]  M. Reno,et al.  Prompt atmospheric neutrino fluxes: perturbative QCD models and nuclear effects , 2016, 1607.00193.

[15]  T. Gaisser,et al.  Sibyll with charm , 2011, 1102.5705.

[16]  E. Avrett,et al.  Structure of the Solar Chromosphere. Basic Computations and Summary of the Results , 1973 .

[17]  Todor Stanev,et al.  Cosmic ray energy spectrum from measurements of air showers , 2013, 1303.3565.

[18]  T. Gaisser,et al.  Signatures of cosmic-ray interactions on the solar surface , 1991 .

[19]  J. Linker,et al.  A Comparison between Global Solar Magnetohydrodynamic and Potential Field Source Surface Model Results , 2006 .

[20]  J. Ferguson,et al.  NEW SOLAR COMPOSITION: THE PROBLEM WITH SOLAR MODELS REVISITED , 2009, 0909.2668.

[21]  T. Gaisser,et al.  Calculation of conventional and prompt lepton fluxes at very high energy , 2015, 1503.00544.

[22]  S. Solanki,et al.  The magnetic field in the solar atmosphere , 2014, 1410.4214.

[23]  T. Gaisser,et al.  Charm production in SIBYLL , 2015, 1502.06353.

[24]  J. Silk,et al.  The photino, the sun, and high-energy neutrinos. , 1985, Physical review letters.

[25]  T. Schwetz,et al.  Updated fit to three neutrino mixing: exploring the accelerator-reactor complementarity , 2016, Journal of High Energy Physics.

[26]  John F. Beacom,et al.  First observation of time variation in the solar-disk gamma-ray flux with Fermi , 2015, 1508.06276.

[27]  Gino Tosti,et al.  FERMI LARGE AREA TELESCOPE OBSERVATIONS OF TWO GAMMA-RAY EMISSION COMPONENTS FROM THE QUIESCENT SUN , 2011 .

[28]  W. Press,et al.  Capture by the sun of a galactic population of weakly interacting massive particles , 1985 .

[29]  L. Bergstrom,et al.  DarkSUSY: Computing Supersymmetric Dark Matter Properties Numerically , 2004 .

[30]  J. Chiang,et al.  FERMI LARGE AREA TELESCOPE OBSERVATIONS OF TWO GAMMA-RAY EMISSION COMPONENTS FROM THE QUIESCENT SUN , 2011, 1104.2093.

[31]  N. Grevesse,et al.  Standard Solar Composition , 1998 .

[32]  A. Fedynitch,et al.  Solar atmospheric neutrinos and the sensitivity floor for solar dark matter annihilation searches , 2017, 1703.07798.

[33]  J. Edsjö,et al.  Limits on the WIMP-nucleon scattering cross-section from neutrino telescopes , 2009 .

[34]  Thunman,et al.  High energy neutrino production by cosmic ray interactions in the Sun. , 1996, Physical review. D, Particles and fields.

[35]  John F. Beacom,et al.  Solar Atmospheric Neutrinos: A New Neutrino Floor for Dark Matter Searches , 2017, 1703.10280.

[36]  Yuhong Fan.  Magnetic Fields in the Solar Convection Zone , 2009 .

[37]  Eugene H. Avrett,et al.  Structure of the solar chromosphere. III. Models of the EUV brightness components of the quiet sun , 1981 .

[38]  Fletcher,et al.  SIBYLL: An event generator for simulation of high energy cosmic ray cascades. , 1994, Physical review. D, Particles and fields.

[39]  M. Reno,et al.  Perturbative charm production and the prompt atmospheric neutrino flux in light of RHIC and LHC , 2015, Proceedings of 40th International Conference on High Energy physics — PoS(ICHEP2020).

[40]  I. Moskalenko,et al.  Very high-energy neutrinos from the Sun , 1993 .

[41]  S. Sarkar,et al.  The prompt atmospheric neutrino flux in the light of LHCb , 2015, Journal of High Energy Physics.

[42]  CTEQ6 parton distributions with heavy quark mass effects , 2003, hep-ph/0307022.