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20072026
most citedLight Sterile Neutrinos: A White Paper

454 citations · 2.2k across the 46 of their papers we have counts for

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Showing 2012 · hep-phShow all

6 papers · 2 filters

hep-ph2012★ 42 cited

Implications of the Pseudo-Dirac Scenario for Ultra High Energy Neutrinos from GRBs

Arman Esmaili, Yasaman Farzan

The source of Ultra High Energy Cosmic Rays (UHECR) is still an unresolved mystery. Up until recently, sources of Gamma Ray Bursts (GRBs) had been considered as a suitable source f…

hep-ph2012★ 32 cited

Kinematical Test of Large Extra Dimension in Beta Decay Experiments

Victor S. Basto-Gonzalez, Arman Esmaili, Orlando L. G. Peres

The forthcoming experiments on neutrino mass measurement using beta decay, open a new window to explore the Large Extra Dimension model. The Kaluza-Klein tower of neutrinos in Larg…

hep-ph2012★ 89 cited

Probing the stability of superheavy dark matter particles with high-energy neutrinos

Arman Esmaili, Alejandro Ibarra, Orlando L. G. Peres

Two of the most fundamental properties of the dark matter particle, the mass and the lifetime, are only weakly constrained by the astronomical and cosmological evidence of dark mat…

hep-ph2012★ 454 cited

Light Sterile Neutrinos: A White Paper

K. N. Abazajian, M. A. Acero, S. K. Agarwalla +184

This white paper addresses the hypothesis of light sterile neutrinos based on recent anomalies observed in neutrino experiments and the latest astrophysical data.

hep-ph2012★ 58 cited

KATRIN Sensitivity to Sterile Neutrino Mass in the Shadow of Lightest Neutrino Mass

Arman Esmaili, Orlando L. G. Peres

The presence of light sterile neutrinos would strongly modify the energy spectrum of the Tritium β-electrons. We perform an analysis of the KATRIN experiment's sensitivity by scann…

hep-ph2012★ 8 cited

Indirect Dark Matter Detection in the Light of Sterile Neutrinos

Arman Esmaili, Orlando L. G. Peres

The recent global fit of short baseline neutrino oscillation data favors the presence of one (or more) sterile neutrino state which leads to new mass splitting Δm^2 ~1 eV^2. We con…