publication . Preprint . Article . 2020

$\chi$aro$\nu$: a tool for neutrino flux generation from WIMPs

Carlos A. Argüelles; Q. R. Liu; J. P. Lazar; Ali Kheirandish;
Open Access English
  • Published: 29 Jul 2020
Abstract
Indirect searches for signatures of corpuscular dark matter have been performed using all cosmic messengers: gamma rays, cosmic rays, and neutrinos. The search for dark matter from neutrinos is of particular importance since they are the only courier that can reach detectors from dark matter processes in dense environments, such as the core of the Sun or Earth, or from the edge of the observable Universe. In this work, we introduce $\chi$aro$\nu$, a software package that, in the spirit of its mythological Greek namesake $\chi \acute\alpha \rho \omega \nu $, bridges the dark sector and Standard Model by predicting neutrino fluxes from different celestial dark mat...
Subjects
arXiv: Astrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::ExperimentAstrophysics::Cosmology and Extragalactic Astrophysics
free text keywords: High Energy Physics - Phenomenology, Astrophysics - High Energy Astrophysical Phenomena, Astronomy and Astrophysics, Particle physics, Flux, Physics, Neutrino
174 references, page 1 of 12

[1] Particle Data Group collaboration, Review of particle physics, Phys. Rev. D 98 (2018) 030001.

[2] I. Esteban, M. C. Gonzalez-Garcia, A. Hernandez-Cabezudo, M. Maltoni and T. Schwetz, Global analysis of three- avour neutrino oscillations: synergies and tensions in the determination of 23; CP , and the mass ordering, JHEP 01 (2019) 106 [1811.05487].

[3] J. N. Bahcall, S. Basu and M. Pinsonneault, How uncertain are solar neutrino predictions?, Phys. Lett. B 433 (1998) 1 [astro-ph/9805135]. [OpenAIRE]

[4] J. N. Bahcall, A. M. Serenelli and S. Basu, New solar opacities, abundances, helioseismology, and neutrino uxes, Astrophys. J. Lett. 621 (2005) L85 [astro-ph/0412440].

[5] R. Davis, A review of the Homestake solar neutrino experiment, Prog. Part. Nucl. Phys. 32 (1994) 13.

[6] J. N. Bahcall, Solving the mystery of the missing neutrinos, physics/0406040.

[7] A. J. Lowe, Neutrino Physics and The Solar Neutrino Problem, 0907.3658.

[8] J. N. Bahcall, M. Gonzalez-Garcia and C. Pena-Garay, Does the sun shine by pp or CNO fusion reactions?, Phys. Rev. Lett. 90 (2003) 131301 [astro-ph/0212331].

[9] J. N. Bahcall, P. Krastev and A. Smirnov, Is large mixing angle MSW the solution of the solar neutrino problems?, Phys. Rev. D 60 (1999) 093001 [hep-ph/9905220]. [OpenAIRE]

[10] F. Zwicky, On the Masses of Nebulae and of Clusters of Nebulae, Astrophysics J. 86 (1937) 271. [OpenAIRE]

[11] F. D. Kahn and L. Woltjer, Intergalactic Matter and the Galaxy, Astrophysics J. 130 (1959) 705.

[12] K. C. Freeman, On the Disks of Spiral and S0 Galaxies, 10.1086/146762 170 (1970) 811.

[13] D. H. Rogstad and G. S. Shostak, Gross properties of ve scd galaxies as determined from 21-centimeter observations, 10.1086/146762 176 (1972) 315.

[14] J. Read, The Local Dark Matter Density, J. Phys. G 41 (2014) 063101 [1404.1938].

[15] Planck collaboration, Planck 2018 results. VI. Cosmological parameters, 1807.06209.

174 references, page 1 of 12
Abstract
Indirect searches for signatures of corpuscular dark matter have been performed using all cosmic messengers: gamma rays, cosmic rays, and neutrinos. The search for dark matter from neutrinos is of particular importance since they are the only courier that can reach detectors from dark matter processes in dense environments, such as the core of the Sun or Earth, or from the edge of the observable Universe. In this work, we introduce $\chi$aro$\nu$, a software package that, in the spirit of its mythological Greek namesake $\chi \acute\alpha \rho \omega \nu $, bridges the dark sector and Standard Model by predicting neutrino fluxes from different celestial dark mat...
Subjects
arXiv: Astrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::ExperimentAstrophysics::Cosmology and Extragalactic Astrophysics
free text keywords: High Energy Physics - Phenomenology, Astrophysics - High Energy Astrophysical Phenomena, Astronomy and Astrophysics, Particle physics, Flux, Physics, Neutrino
174 references, page 1 of 12

[1] Particle Data Group collaboration, Review of particle physics, Phys. Rev. D 98 (2018) 030001.

[2] I. Esteban, M. C. Gonzalez-Garcia, A. Hernandez-Cabezudo, M. Maltoni and T. Schwetz, Global analysis of three- avour neutrino oscillations: synergies and tensions in the determination of 23; CP , and the mass ordering, JHEP 01 (2019) 106 [1811.05487].

[3] J. N. Bahcall, S. Basu and M. Pinsonneault, How uncertain are solar neutrino predictions?, Phys. Lett. B 433 (1998) 1 [astro-ph/9805135]. [OpenAIRE]

[4] J. N. Bahcall, A. M. Serenelli and S. Basu, New solar opacities, abundances, helioseismology, and neutrino uxes, Astrophys. J. Lett. 621 (2005) L85 [astro-ph/0412440].

[5] R. Davis, A review of the Homestake solar neutrino experiment, Prog. Part. Nucl. Phys. 32 (1994) 13.

[6] J. N. Bahcall, Solving the mystery of the missing neutrinos, physics/0406040.

[7] A. J. Lowe, Neutrino Physics and The Solar Neutrino Problem, 0907.3658.

[8] J. N. Bahcall, M. Gonzalez-Garcia and C. Pena-Garay, Does the sun shine by pp or CNO fusion reactions?, Phys. Rev. Lett. 90 (2003) 131301 [astro-ph/0212331].

[9] J. N. Bahcall, P. Krastev and A. Smirnov, Is large mixing angle MSW the solution of the solar neutrino problems?, Phys. Rev. D 60 (1999) 093001 [hep-ph/9905220]. [OpenAIRE]

[10] F. Zwicky, On the Masses of Nebulae and of Clusters of Nebulae, Astrophysics J. 86 (1937) 271. [OpenAIRE]

[11] F. D. Kahn and L. Woltjer, Intergalactic Matter and the Galaxy, Astrophysics J. 130 (1959) 705.

[12] K. C. Freeman, On the Disks of Spiral and S0 Galaxies, 10.1086/146762 170 (1970) 811.

[13] D. H. Rogstad and G. S. Shostak, Gross properties of ve scd galaxies as determined from 21-centimeter observations, 10.1086/146762 176 (1972) 315.

[14] J. Read, The Local Dark Matter Density, J. Phys. G 41 (2014) 063101 [1404.1938].

[15] Planck collaboration, Planck 2018 results. VI. Cosmological parameters, 1807.06209.

174 references, page 1 of 12
Any information missing or wrong?Report an Issue