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We examine the sterile neutrino dark matter production in the primordial plasma with lepton asymmetry unequally distributed over different neutrino flavors. We argue that with the specific flavor fractions, one can mitigate limits from the…

高能物理 - 唯象学 · 物理学 2025-07-29 Dmitry Gorbunov , Dmitry Kalashnikov , George Krugan

We explore resonant production of sterile neutrino dark matter via the Shi-Fuller (SF) mechanism, revisiting its cosmological viability in light of recent results demonstrating that lepton-number asymmetries $L_\alpha \gtrsim 1$ at…

高能物理 - 唯象学 · 物理学 2025-12-22 Cannon M. Vogel , Helena García Escudero , Julien Froustey , Kevork N. Abazajian

We perform an exhaustive scan of the allowed resonant production regime for sterile neutrino dark matter in order to improve constraints for dark matter structures which arise from the non-thermal sterile neutrino energy spectra.…

高能物理 - 唯象学 · 物理学 2017-05-03 John F. Cherry , Shunsaku Horiuchi

It has been proposed that two resonances could coincide in the early universe at temperatures $T \sim 0.2 ... 0.5$ GeV: one between two nearly degenerate GeV-scale sterile neutrinos, producing a large lepton asymmetry through freeze-out and…

高能物理 - 唯象学 · 物理学 2020-07-08 J. Ghiglieri , M. Laine

Lepton flavour asymmetries generated at the onset of the oscillations of sterile neutrinos with masses above the electroweak scale can be large enough to partly survive washout and to explain the baryon asymmetry of the Universe. This opens…

高能物理 - 唯象学 · 物理学 2014-10-01 Bjorn Garbrecht

The putative recent indication of an unidentified 3.55 keV X-ray line in certain astrophysical sources is taken as a motivation for an improved theoretical computation of the cosmological abundance of 7.1 keV sterile neutrinos. If the line…

高能物理 - 唯象学 · 物理学 2015-12-07 J. Ghiglieri , M. Laine

We propose a new and unique dark matter candidate: $\sim 100$ eV to $\sim 10$ keV sterile neutrinos produced via lepton number-driven resonant MSW (Mikheyev-Smirnov-Wolfenstein) conversion of active neutrinos. The requisite lepton number…

天体物理学 · 物理学 2009-10-31 Xiangdong Shi , George M. Fuller

We apply phase-space density considerations to obtain lower bounds on the mass of sterile neutrino as dark matter candidate. The bounds are different for non-resonant production, resonant production in the presence of lepton asymmetry and…

高能物理 - 唯象学 · 物理学 2009-12-04 D. Gorbunov , A. Khmelnitsky , V. Rubakov

We consider the leptonic asymmetry generation in the nuMSM via hadronic decays of sterile neutrinos at T<<T_{EW}, when the masses of two heavier sterile neutrinos are between pion mass and 2 GeV. The choice of upper mass bound is motivated…

高能物理 - 唯象学 · 物理学 2013-09-25 Volodymyr M. Gorkavenko , Igor Rudenok , Stanislav I. Vilchynskiy

It has been proposed that in a part of the parameter space of the Standard Model completed by three generations of keV...GeV right-handed neutrinos, neutrino masses, dark matter, and baryon asymmetry can be accounted for simultaneously.…

高能物理 - 唯象学 · 物理学 2019-07-25 J. Ghiglieri , M. Laine

Previous fits of sterile neutrino dark matter models to cosmological data assumed a peculiar production mechanism, which is not representative of the best-motivated particle physics models given current data on neutrino oscillations. These…

高能物理 - 唯象学 · 物理学 2009-06-30 Alexey Boyarsky , Julien Lesgourgues , Oleg Ruchayskiy , Matteo Viel

To explain the dark matter and the baryon asymmetry of the Universe, the parameters of the $\nu$MSM (an extension of the Minimal Standard Model by three singlet neutrinos with masses smaller than the electroweak scale) must be fine-tuned:…

高能物理 - 唯象学 · 物理学 2008-11-26 Mikhail Shaposhnikov

We consider heavy sterile neutrinos $\nu_s$, with mass in the range 10 MeV $\lesssim m_s \lesssim m_{\pi} \sim 135$ MeV, thermally produced in the early universe and freezing out after the QCD phase transition. The existence of these…

高能物理 - 唯象学 · 物理学 2022-02-24 L. Mastrototaro

We explore the range of parameters for dark-matter sterile neutrinos in an extention of the Minimal Standard Model by three singlet fermions with masses below the electroweak scale (the $\nu$MSM). This simple model can explain a wide range…

高能物理 - 唯象学 · 物理学 2008-11-26 Takehiko Asaka , Mikhail Shaposhnikov , Alexander Kusenko

An extension of the Standard Model by three right-handed neutrinos with masses smaller than the electroweak scale (the $\nu$MSM) can explain simultaneously dark matter and baryon asymmetry of the Universe, being consistent with the data on…

天体物理学 · 物理学 2016-11-15 Mikhail Shaposhnikov

The existence of a large primordial neutrino asymmetry is an intriguing possibility, both observationally and theoretically. Such an asymmetry can lead to the resonant production of $\mathrm{keV}$-scale sterile neutrinos, which are a…

高能物理 - 唯象学 · 物理学 2025-10-08 Kentaro Kasai , Masahiro Kawasaki , Kai Murai

We study the contribution of massive dominantly sterile neutrinos, $N$, to the Lepton Number and Lepton Flavor Violating semileptonic decays of $\tau$ and $B, D, K$-mesons. We focus on special domains of sterile neutrino masses $m_{N}$…

高能物理 - 唯象学 · 物理学 2013-08-27 Juan Carlos Helo , Sergey Kovalenko , Ivan Schmidt

We consider the possibility of simultaneously addressing the baryon asymmetry of the Universe, the dark matter problem and the neutrino mass generation in minimal extensions of the Standard Model via sterile fermions with (small) total…

高能物理 - 唯象学 · 物理学 2018-03-20 Asmaa Abada , Giorgio Arcadi , Valerie Domcke , Michele Lucente

We study sterile neutrino dark matter (DM) in a classically conformal U(1)' extension of the Standard Model with three right-handed neutrinos and a Majoron-like singlet scalar that generate the observed pattern of active neutrino masses and…

高能物理 - 唯象学 · 物理学 2026-02-13 João Gonçalves , Danny Marfatia , António P. Morais , Vinícius Oliveira , Roman Pasechnik

We investigate quantitatively the extent to which having a primordial leptonic asymmetry (n_nu \neq n_nubar) relaxes the bounds on light sterile neutrinos imposed by BBN and LSS. We adopt a few assumptions that allow us to solve the…

天体物理学 · 物理学 2008-11-26 Yi-Zen Chu , Marco Cirelli
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