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200 papers

Distortions of CMB temperature and polarization anisotropy maps caused by gravitational lensing, observable with high angular resolution and sensitivity, can be used to constrain the sterile neutrino mass, offering several advantages…

Astrophysics · Physics 2009-06-23 L. A. Popa , A. Vasile

We study the effects of neutrino spin-flip in the magnetic field, B_{AGN}, of active galactic nuclei (AGN) for high-energy neutrinos (E > 10^{6} GeV) originating from AGN induced by an interplay of the violation of equivalence principle…

High Energy Physics - Phenomenology · Physics 2010-12-03 M. Anwar Mughal , H. Athar

It is commonly assumed that the cosmological and astrophysical bounds on the mixings of sterile with active neutrinos are much more stringent than those obtained from laboratory measurements. We point out that in scenarios with a very low…

Astrophysics · Physics 2009-06-23 Graciela Gelmini , Efunwande Osoba , Sergio Palomares-Ruiz , Silvia Pascoli

For the first time the antineutrino spectrum formed as a result of neutron and tritium decays during the epoch of primordial nucleosynthesis is calculated. This spectrum is a non-thermal increase in addition to the standard cosmic neutrino…

Cosmology and Nongalactic Astrophysics · Physics 2018-10-05 Alexandre V. Ivanchik , Vlad Yu. Yurchenko

In the standard model neutrinos are assumed to have streamed across the Universe since they last scattered at the weak decoupling epoch when the temperature of the standard-model plasma was ~MeV. The shear stress of free-streaming neutrinos…

Cosmology and Nongalactic Astrophysics · Physics 2015-01-07 Francis-Yan Cyr-Racine , Kris Sigurdson

Distortions of CMB temperature and polarization maps caused by gravitational lensing, observable with high angular resolution and sensitivity, can be used to constrain the sterile neutrino mass, m_s, from CMB data alone. We forecast…

Astrophysics · Physics 2007-05-23 L. A. Popa , A. Vasile

We study the nonresonant oscillations between left-handed electron neutrinos nu_e and nonthermalized sterile neutrinos nu_s in the early Universe plasma. The case when nu_s do not thermalize till 2 MeV and the oscillations become effective…

High Energy Physics - Phenomenology · Physics 2011-02-24 D. P. Kirilova , M. V. Chizhov

In light of the recent BICEP2 B-mode polarization detection, which implies a large inflationary tensor-to-scalar ratio r_{0.05}=0.2^{+0.07}_{-0.05}, we re-examine the evidence for an extra sterile massive neutrino, originally invoked to…

Cosmology and Nongalactic Astrophysics · Physics 2014-10-08 Cora Dvorkin , Mark Wyman , Douglas H. Rudd , Wayne Hu

The LHAASO collaboration has reported their observation of very high energy photons ($E^{max}_\gamma \simeq 18$ TeV) from the gamma-ray burst GRB221009A. The sterile neutrino that involves both mixing and transition magnetic moment may be a…

High Energy Physics - Phenomenology · Physics 2023-07-26 Shu-Yuan Guo , Maxim Khlopov , Lei Wu , Bin Zhu

We derive here a robust bound on the effective number of neutrinos from constraints on primordial nucleosynthesis yields of deuterium and helium. In particular, our results are based on very weak assumptions on the astrophysical…

Cosmology and Nongalactic Astrophysics · Physics 2011-06-13 Gianpiero Mangano , Pasquale D. Serpico

Late-decaying particles naturally arise in many extensions of the Standard Model, directly impacting key cosmological processes in the early universe, such as Big Bang Nucleosynthesis (BBN). BBN studies often consider electromagnetic energy…

High Energy Physics - Phenomenology · Physics 2025-01-17 Lucia Angel , Giorgio Arcadi , Matheus M. A. Paixão , Farinaldo S. Queiroz

Although the MiniBooNE experiment has severely restricted the possible existence of light sterile neutrinos, a few anomalies persist in oscillation data, and the possibility of extra light species contributing as a subdominant hot (or warm)…

Astrophysics · Physics 2010-04-23 Mario A. Acero , Julien Lesgourgues

We analyse the process of reheating the Universe in the electroweak theory where the Higgs field plays a role of the inflaton. We estimate the maximal temperature of the Universe and fix the initial conditions for radiation-dominated phase…

High Energy Physics - Phenomenology · Physics 2010-04-14 F. Bezrukov , D. Gorbunov , M. Shaposhnikov

Sterile neutrinos are possible dark matter candidates. We examine here possible detection mechanisms, assuming that the neutrino has a mass of about 50 keV and couples to the ordinary neutrino. Even though this neutrino is quite heavy, it…

High Energy Physics - Phenomenology · Physics 2018-09-25 Paraskevi C. Divari , John D. Vergados

We analyze the influence of decaying sterile neutrinos with the masses in the range 1-140 MeV on the primordial Helium-4 abundance, explicitly solving the Boltzmann equations for all particle species, taking into account neutrino flavour…

High Energy Physics - Phenomenology · Physics 2012-10-11 Oleg Ruchayskiy , Artem Ivashko

We investigate the effects of strong magnetic fields on the equation of state of warm stellar matter as it may occur in a protoneutron star. Both neutrino free and neutrino trapped matter at a fixed entropy per baryon are analyzed. A…

Nuclear Theory · Physics 2015-05-28 A. Rabhi , P. K. Panda , C. Providência

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 \Delta m^2 ~1 eV^2. We consider the effect of this new states on the evolution…

High Energy Physics - Phenomenology · Physics 2012-07-02 Arman Esmaili , Orlando L. G. Peres

It is shown that the future SNO and Super-Kamiokande experiments, in which high energy $^8\mathrm{B}$ neutrinos will be detected through the observation of CC, NC and $\nu$--$e$ elastic scattering processes, could allow to reveal in a model…

High Energy Physics - Phenomenology · Physics 2009-09-25 S. M. Bilenky , C. Giunti

The magnetic field in the convective zone of the Sun has a random small-scale component with the r.m.s. value substantially exceeding the strength of a regular large-scale field. For two Majorana neutrino flavors $\times$ two helicities in…

High Energy Physics - Phenomenology · Physics 2009-10-31 A. A. Bykov , V. Yu. Popov , A. I. Rez , V. B. Semikoz , D. D. Sokoloff

We show that when the neutrino minimal standard model ($\nu MSM$) with a light sterile neutrino has a long range interaction between the neutrino vacuum charge density and a dark U(1) gauge potential, late time acceleration is dynamically…

High Energy Physics - Phenomenology · Physics 2013-06-14 Stephon H. S. Alexander