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Taking into account new physics and astronomy developments I give a revised high energy neutrino flux for the AGN core model of Stecker, Done, Salamon and Sommers

Astrophysics · Physics 2009-11-13 F. W. Stecker

We study the gravitational scattering of ultrarelativistic neutrinos off a rotating supermassive black hole (BH) surrounded by a thick magnetized accretion disk. Neutrinos interact electroweakly with background matter and with the magnetic…

High Energy Astrophysical Phenomena · Physics 2023-09-20 Maxim Dvornikov

A correlation between the highest energy Cosmic Rays (above ~ EeV) and the distribution of active galactic nuclei (AGN) gives rise to a prediction of neutrino production in the same sources. In this paper, we present a detailed AGN model,…

Astrophysics · Physics 2009-11-13 Julia K. Becker , Peter L. Biermann

Since decoupling in the early universe in helicity states, primordial neutrinos propagating in astrophysical magnetic fields precess and undergo helicity changes. In view of the XENON1T experiment possibly finding a large magnetic moment of…

High Energy Physics - Phenomenology · Physics 2021-05-19 Gordon Baym , Jen-Chieh Peng

We study the onset of neutron drip in high density matter in the presence of magnetic field. It has been found that for systems having only protons and electrons, in the presence of magnetic field >~ 10^{15}G, the neutronization occurs at a…

Solar and Stellar Astrophysics · Physics 2015-06-19 M. V. Vishal , Banibrata Mukhopadhyay

We consider the centrifugal acceleration of charged test particles by rotating magnetospheres which are widely believed to be responsible for the relativistic jet phenomenon in active galactic nuclei (AGN). Based on an analysis of forces…

Astrophysics · Physics 2007-05-23 F. M. Rieger , K. Mannheim

Spin oscillations of neutrinos, gravitationally scattered off a black hole (BH), are studied. The cases of nonrotating and rotating BHs are analyzed. We derive the analytic expressions for the transition and survival probabilities of spin…

High Energy Physics - Phenomenology · Physics 2020-06-03 Maxim Dvornikov

Production of the expected high energy neutrino flux with energy greater than tens of thousands of GeV in some astrophysical sites such as the galactic plane as well as the centers of some distant galaxies is reviewed. The expected changes…

High Energy Physics - Phenomenology · Physics 2007-05-23 H. Athar

We investigate the effect of a strong magnetic field on the structure of neutron stars in a model with perturbative $f(R)$ gravity. The effect of an interior strong magnetic field of about $10^{17 \sim 18}$ G on the equation of state is…

High Energy Astrophysical Phenomena · Physics 2015-06-15 Myung-Ki Cheoun , Cemsinan Deliduman , Can Güngör , Vildan Keleş , C. Y. Ryu , Toshitaka Kajino , Grant J. Mathews

We investigate the effect of the density-dependent proton and neutron gaps on vortex dynamics in neutron stars. We argue that the persistence of neutron star magnetic fields on timescales of $10^9$ y suggests a superconducting gap curve…

Nuclear Theory · Physics 2009-10-31 Stephen D. H. Hsu

Growing supermassive black holes (Active Galactic Nuclei; AGN) release energy with the potential to alter their host galaxies and larger-scale environment; a process named "AGN feedback". Feedback is a required component of galaxy formation…

Astrophysics of Galaxies · Physics 2024-04-15 Chris M. Harrison , Cristina Ramos Almeida

Oscillations of neutrinos $\nu_L \leftrightarrow \nu_R$ in presence of an arbitrary electromagnetic field are considered. We introduce the Hamiltonian for the neutrino spin evolution equation that accounts for possible effects of…

High Energy Physics - Phenomenology · Physics 2009-10-31 A. M. Egorov , A. E. Lobanov , A. I. Studenikin

Recent reports of possible correlations between high energy neutrinos observed by IceCube and Active Galactic Nuclei (AGN) activity sparked a burst of publications that attempt to predict the neutrino flux of these sources. However, often…

High Energy Astrophysical Phenomena · Physics 2018-04-04 S. Richter , F. Spanier

The cross section for neutrino helicity spin-flip obtained from a new f(R, T) model of gravitation with dynamic torsion field introduced by one of the authors in [1], is phenomenologically analyzed. To this end, due to the logarithmical…

High Energy Physics - Phenomenology · Physics 2017-03-08 David Alvarez-Castillo , Diego Julio Cirilo-Lombardo , Jilberto Zamora-Saa

The viscosity-driven "spin-flip" instability in newborn magnetars with interior toroidal magnetic fields is re-examined. We calculate the bulk viscosity coefficient ($\zeta$) of cold, $npe \mu$ matter in neutron stars (NS), for selected…

High Energy Astrophysical Phenomena · Physics 2018-07-18 Simone Dall'Osso , Luigi Stella , Cristiano Palomba

Flavor oscillations of neutrinos are analyzed in the framework of Brans-Dicke theory of gravity. We find a shift of quantum mechanical phase of neutrino proportional to $G_N\Delta m^2$ and depending on the parameter $\omega$. Consequences…

General Relativity and Quantum Cosmology · Physics 2010-11-19 S. Capozziello , G. Lambiase

Neutrino spin and flavour oscillation in curved spacetime have been studied for the most general static spherically symmetric configuration. Using the symmetry properties we have derived spin oscillation frequency for neutrino moving along…

General Relativity and Quantum Cosmology · Physics 2015-10-16 Sumanta Chakraborty

Neutrino asymmetry generation from active-sterile neutrino oscillations in the early Universe has different important cosmological effects. We discuss its basic features and present recent results on the borders of the generation for mixing…

High Energy Physics - Phenomenology · Physics 2007-05-23 P. Di Bari

Relic neutrinos from the Big Bang decoupled from the hot plasma predominantly in helicity eigenstates. Their subsequent propagation through gravitational inhomogeneities of the Universe alters the helicities of both Dirac and Majorana…

High Energy Physics - Phenomenology · Physics 2021-11-01 Gordon Baym , Jen-Chieh Peng

The main fuelling processes for Active Galactic Nuclei (AGN) are currently unknown. Previous work showed that galaxies with a large kinematic misalignment between their stellar and gas reservoirs have a higher AGN fraction than galaxies…