English
Related papers

Related papers: Particle Physics on Ice: Constraints on Neutrino I…

200 papers

A search for extremely high energy cosmic neutrinos has been carried out with the IceCube Neutrino Observatory. The main signals in the search are neutrino-induced energetic charged leptons and their rate depends on the neutrino-nucleon…

High Energy Physics - Phenomenology · Physics 2010-12-23 Shigeru Yoshida

New physics beyond the electroweak scale may increase weak interaction cross sections beyond the Standard Model predictions. Such cross sections can be expected within theories that solve the hierarchy problem of known interactions with a…

High Energy Physics - Phenomenology · Physics 2009-10-31 Craig Tyler , Angela V. Olinto , Guenter Sigl

A number of experimental techniques are currently being deployed in an effort to make the first detection of ultra-high energy cosmic neutrinos. To accomplish this goal, techniques using radio and acoustic detectors are being developed,…

Astrophysics · Physics 2008-11-26 Francis Halzen , Dan Hooper

The energy at which cosmic rays from extra-galactic sources begin to dominate over those from galactic sources is an important open question in astroparticle physics. A natural candidate is the energy at the 'ankle' in the approximately…

High Energy Astrophysical Phenomena · Physics 2014-11-18 Markus Ahlers , Luis A. Anchordoqui , Subir Sarkar

We begin with a brief overview of highest-energy cosmic ray data, and the experiments which will perform neutrino astronomy. We then discuss two particle physics aspects of neutrinos. They are possible long-lifetime decay of the neutrino,…

Astrophysics · Physics 2011-07-19 Thomas J. Weiler

The astrophysical neutrinos recently discovered by the IceCube neutrino telescope have the highest detected neutrino energies --- from TeV to PeV --- and travel the longest distances --- up to a few Gpc, the size of the observable Universe.…

High Energy Astrophysical Phenomena · Physics 2020-12-30 Mauricio Bustamante

Neutrino astrophysics offers new perspectives on the Universe investigation: high energy neutrinos, produced by the most energetic phenomena in our Galaxy and in the Universe, carry complementary (if not exclusive) information about the…

High Energy Astrophysical Phenomena · Physics 2010-02-11 T. Chiarusi , M. Spurio

Astrophysical neutrinos are expected to be produced in the interactions of ultra-high energy cosmic-rays with surrounding photons. The fluxes of the astrophysical neutrinos are highly dependent on the characteristics of the cosmic-ray…

High Energy Astrophysical Phenomena · Physics 2015-06-04 Shigeru Yoshida , Aya Ishihara

With the discovery of evidence for neutrino mass, a vivid gamma ray sky at multi-TeV energies, and cosmic ray particles with unexpectedly high energies, astroparticle physics currently runs through an era of rapid progress and moving…

Astrophysics · Physics 2010-12-03 Karl Mannheim

IceCube, a cubic kilometer neutrino telescope will be capable of probing neutrino-nucleon interactions in the ultrahigh energy regime, far beyond the energies reached by colliders. In this article we introduce a new observable that combines…

High Energy Physics - Phenomenology · Physics 2008-11-26 Matias M. Reynoso , Oscar A. Sampayo

We review the prospects for probing new physics with neutrino astrophysics. High energy neutrinos provide an important means of accessing physics beyond the electroweak scale. Neutrinos have a number of advantages over conventional…

High Energy Physics - Phenomenology · Physics 2008-12-18 Nicole F. Bell

The astrophysical neutrinos discovered by IceCube have the highest detected neutrino energies --- from TeV to PeV --- and likely travel the longest distances --- up to a few Gpc, the size of the observable Universe. These features make them…

High Energy Astrophysical Phenomena · Physics 2019-07-23 Carlos A. Argüelles , Mauricio Bustamante , Ali Kheirandish , Sergio Palomares-Ruiz , Jordi Salvado , Aaron C. Vincent

In recent years precision cosmology has become an increasingly powerful probe of particle physics. Perhaps the prime example of this is the very stringent cosmological upper bound on the neutrino mass. However, other aspects of neutrino…

Cosmology and Nongalactic Astrophysics · Physics 2022-03-02 Steen Hannestad

Astrophysical neutrinos travel long distances from their sources to the Earth traversing dark matter halos of clusters of galaxies and that of our own Milky Way. The interaction of neutrinos with dark matter may affect the flux of…

Cosmology and Nongalactic Astrophysics · Physics 2019-05-08 Ki-Young Choi , Jongkuk Kim , Carsten Rott

Cosmic rays have been observed up to energies $10^8$ times larger than those of the best particle accelerators. Studies of astrophysical particles (hadrons, neutrinos and photons) at their highest observed energies have implications for…

Astrophysics · Physics 2009-11-10 F. W. Stecker

With the discovery of a high-energy neutrino flux in the 0.1 PeV to PeV range from beyond the Earth's atmosphere with the IceCube detector, neutrino astronomy has achieved a major breakthrough in the exploration of the high-energy universe.…

High Energy Astrophysical Phenomena · Physics 2019-08-13 A. Kappes

Recent international efforts have brought us closer to unveiling the century old mystery of the origin of cosmic rays. Cosmic ray, gamma ray, and neutrino observatories are reaching the necessary sensitivity to study the highest energy…

High Energy Astrophysical Phenomena · Physics 2012-03-16 Angela V. Olinto

Kilometer-scale neutrino detectors such as IceCube are discovery instruments covering nuclear and particle physics, cosmology and astronomy. Examples of their multidisciplinary missions include the search for the particle nature of dark…

Astrophysics · Physics 2007-05-23 F. Halzen

We elucidate the physical basis for the upper bound on high energy neutrino fluxes implied by the observed cosmic ray flux. We stress that the bound is valid for neutrinos produced either by p,gamma reactions or by p-p(n) reactions in…

High Energy Physics - Phenomenology · Physics 2011-04-20 John Bahcall , Eli Waxman
‹ Prev 1 2 3 10 Next ›