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相关论文: Neutrino spin-flip effects in active galactic nucl…

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Evidence for high-energy astrophysical PeV neutrinos has been found in the IceCube experiment from an analysis with a 7.5 year (2010 - 2017) data. Active galactic nuclei (AGN) are among the most prominent objects in the universe, and are…

高能天体物理现象 · 物理学 2022-03-08 Rajat K. Dey , Animesh Basak , Sabyasachi Ray

We investigate the production of magnetic flux from rotating black holes in active galactic nuclei (AGNs) and compare it with the upper limit of ultrahigh energy cosmic ray (UHECR) luminosities, calculated from observed integral flux of…

高能天体物理现象 · 物理学 2015-11-04 C. H. Coimbra-Araújo , R. C. Anjos

A new type of electromagnetic radiation by a neutrino with non-zero magnetic (and/or electric) moment moving in background matter and electromagnetic field is considered. This radiation originates from the quantum spin flip transitions and…

高能物理 - 唯象学 · 物理学 2009-11-07 A. Lobanov , A. Studenikin

Active Galactic Nuclei (AGN) are known to show flux variability over all observable timescales and across the entire electromagnetic spectrum. Over the past decade, a growing number of sources have been observed to show dramatic flux and…

星系天体物理 · 物理学 2022-11-11 Claudio Ricci , Benny Trakhtenbrot

The inclusion of massive neutrinos affects the cross sections involved in the formation of heavy nuclei, modifying their abundances. Rapid neutron capture processes (r-process) are often associated with explosive events such as…

高能物理 - 唯象学 · 物理学 2018-09-10 M. M. Saez , M. E. Mosquera , O. Civitarese

We present a series of cosmological magnetohydrodynamic (MHD) simulations that simultaneously follow the formation of a galaxy cluster and evolution of magnetic fields ejected by an Active Galactic Nucleus (AGN). Specifically, we…

宇宙学与河外天体物理 · 物理学 2015-05-20 Hao Xu , Hui Li , David C. Collins , Shengtai Li , Michael L. Norman

Active Galactic Nuclei (AGNs) emit substantial fluxes of high-energy electromagnetic radiation, and have therefore attracted some recent attention for their negative impact on galactic habitability. In this paper, we propose that AGNs may…

地球与行星天体物理 · 物理学 2019-05-28 Manasvi Lingam , Idan Ginsburg , Shmuel Bialy

We study the propagation of neutrinos from compact astrophysical objects with strong magnetic field, such as magnetars. Both neutrino spin rotation and oscillations in a realistic three-flavor model are taken into account. We solve the…

高能物理 - 唯象学 · 物理学 2020-12-08 A. V. Chukhnova , A. E. Lobanov

The neutrino force results from the exchange of a pair of neutrinos. A neutrino background can significantly influence this force. In this work, we present a comprehensive calculation of the neutrino force in various neutrino backgrounds…

高能物理 - 唯象学 · 物理学 2025-10-10 Mitrajyoti Ghosh , Yuval Grossman , Walter Tangarife , Xun-Jie Xu , Bingrong Yu

We test the recently proposed idea that outflows associated with Active Galactic Nuclei (AGN) could be neutrino emitters in two complementary ways. First, we cross-correlate a list of 94 "bona fide" AGN outflows with the most complete and…

高能天体物理现象 · 物理学 2018-04-25 P. Padovani , A. Turcati , E. Resconi

We discuss the excitation of sterile neutrinos in the early universe using general quantum kinetic equations, which also incorporate a possible primordial magnetic field $B$. We find a new contribution to the excitation propability, which…

高能物理 - 唯象学 · 物理学 2009-10-28 Kari Enqvist , Jukka Maalampi , V. B. Semikoz

Neutrinos can be pseudo-Dirac in Nature - they can be Majorana fermions while behaving effectively as Dirac fermions. Such scenarios predict active-sterile neutrino oscillations driven by a tiny mass-squared difference $(\delta m^2)$, which…

高能物理 - 唯象学 · 物理学 2024-03-18 Thomas Rink , Manibrata Sen

In astrophysical environments, neutrinos may propagate over a long distance in a magnetic field. In the presence of a rotating magentic field, the neutrino spin can flip from left-handed neutrino to right-handed neutrino. Smirnov…

量子物理 · 物理学 2015-12-31 Da-Bao Yang , Ji-Xuan Hou , Ku Meng

Light sterile neutrinos can be excited by oscillations with active neutrinos in the early universe. Their properties can be constrained by their contribution as extra-radiation, parameterized in terms of the effective number of neutrino…

宇宙学与河外天体物理 · 物理学 2015-06-15 Alessandro Mirizzi , Gianpiero Mangano , Ninetta Saviano , Enrico Borriello , Carlo Giunti , Gennaro Miele , Ofelia Pisanti

We suggest that the presence of a quantum gravity induced minimal length can be explored using neutrino oscillation probabilities. Neutrinos seem ideally suited for this investigation because they can propagate freely over large distances…

高能物理 - 唯象学 · 物理学 2011-11-21 Martin Sprenger , Piero Nicolini , Marcus Bleicher

We study the CMB anisotropy induced by the non-linear perturbations in the massive neutrino density associated to the non-linear gravitational clustering proceses. Our results show that for the neutrino fraction in agreement with that…

天体物理学 · 物理学 2009-11-07 L. A. Popa , C. Burigana , N. Mandolesi

The energetic feedback from supermassive black holes can influence star formation at the centres of galaxies. Observational evidence for active galactic nucleus (AGN) impact on star formation can be searched for in galaxies by combining…

星系天体物理 · 物理学 2022-11-14 Prajwel Joseph , Koshy George , K. T. Paul

We show that the flip-flop transitions in X-ray binaries (rapid cycling between different spectral states which are sometimes seen near the global state transition) show a series of analogies to the changing state phenomena (rapid changes…

We derive an effective neutrino evolution Hamiltonian and corresponding expression for neutrino spin oscillations probabilities accounting for neutrino interactions with external electric current due to neutrino charge radii and anapole…

高能物理 - 唯象学 · 物理学 2023-02-13 Vadim Shakhov , Alexander Studenikin

We calculate the nucleon contribution to the electromagnetic vertex of a neutrino in a background of particles, including the effect of the anomalous magnetic moment of the nucleons. Explicit formulas for the form factors are given in…

高能物理 - 唯象学 · 物理学 2009-10-30 Juan Carlos D'Olivo , Jose F. Nieves