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We study a light dark matter in a radiative neutrino model to explain the X-ray line signal at about $3.5$ keV recently reported by XMN-Newton X-ray observatory using data of various galaxy clusters and Andromeda galaxy. The signal requires…

高能物理 - 唯象学 · 物理学 2014-03-21 Seungwon Baek , Hiroshi Okada

We study the phenomenology of a keV sterile neutrino in a supersymmetric model with $U(1)_R-$ lepton number in the light of a very recent observation of an X-ray line signal at around 3.5 keV, detected in the X-ray spectra of Andromeda…

高能物理 - 唯象学 · 物理学 2015-06-19 Sabyasachi Chakraborty , Dilip Kumar Ghosh , Sourov Roy

The recently discovered X-ray line at about $3.5\,$keV can be explained by sterile neutrino dark matter with mass, $m_s \simeq 7\,$keV, and the mixing, $\sin^2 2\theta \sim 10^{-10}$. Such sterile neutrino is more long-lived than estimated…

高能物理 - 唯象学 · 物理学 2015-06-18 Hiroyuki Ishida , Kwang Sik Jeong , Fuminobu Takahashi

Recent reports of a weak unidentified emission line at ~3.5 keV found in spectra of several matter-dominated objects may give a clue to resolve the long-standing problem of dark matter. One of the best physically motivated particle…

宇宙学与河外天体物理 · 物理学 2016-06-14 Anton Rudakovskyi , Dmytro Iakubovskyi

We present some R-parity conserving supersymmetric models which can accommodate the 3.5 keV X-ray line reported in recent spectral studies of the Perseus galaxy cluster and the Andromeda galaxy. Within the Minimal Supersymmetric Standard…

高能物理 - 唯象学 · 物理学 2015-06-22 Bhaskar Dutta , Ilia Gogoladze , Rizwan Khalid , Qaisar Shafi

One of possible explanations of a faint narrow emission line at 3.5 keV reported in our Galaxy, Andromeda galaxy and a number of galaxy clusters is the dark matter made of 7 keV sterile neutrinos. Another signature of such sterile neutrino…

宇宙学与河外天体物理 · 物理学 2018-11-28 Anton Rudakovskyi , Dmytro Iakubovskyi

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 explore the possibility of light and superlight sterile neutrinos in the recently proposed Minimal Radiative Inverse Seesaw extension of the Standard Model for neutrino masses, in which all existing neutrino data can be explained. In…

高能物理 - 唯象学 · 物理学 2013-08-01 P. S. Bhupal Dev , Apostolos Pilaftsis

The recent discovery of unexplained X-ray line of $3.5-3.6$ keV emitted from the Perseus cluster of galaxies and M31 and the excess X-ray line of $8.7$ keV emitted from the Milky Way center may indicate that dark matter would decay. In this…

高能天体物理现象 · 物理学 2016-04-07 Man Ho Chan

Motivated by the recent observations on sterile neutrinos, we present a minimal extension of the canonical type-I seesaw by adding one extra singlet fermion. After the decoupling of right-handed neutrinos, an eV-scale mass eigenstate is…

高能物理 - 唯象学 · 物理学 2015-06-03 He Zhang

Sterile neutrinos with masses in the keV range are viable candidates for the warm dark matter. We analyze existing data for the extragalactic diffuse X-ray background for signatures of sterile neutrino decay. The absence of detectable…

天体物理学 · 物理学 2009-11-11 A. Boyarsky , A. Neronov , O. Ruchayskiy , M. Shaposhnikov

We explore the possibility of a single generation of $keV$ scale sterile neutrino ($m_S$) as a dark matter candidate within the minimal extended seesaw (MES) framework and it's influence in neutrinoless double beta decay ($0\nu\beta\beta$)…

高能物理 - 唯象学 · 物理学 2020-08-26 Pritam Das , Mrinal Kumar Das

Left-Right Symmetric Model(LRSM) in this work is extended with a sterile fermion per generation, the lightest of the same is considered to be a suitable dark matter candidate for the study and analysis of the associated properties. The…

高能物理 - 唯象学 · 物理学 2026-01-07 Ankita Kakoti , Mrinal Kumar Das

Sterile neutrinos are natural extensions to the standard model of particle physics in neutrino mass generation mechanisms. If they are relatively light, less than approximately 10 keV, they can alter cosmology significantly, from the early…

高能物理 - 唯象学 · 物理学 2018-12-19 Kevork N. Abazajian

We study the possibility of simultaneously addressing neutrino phenomenology and the dark matter in the framework of inverse seesaw. The model is the extension of the standard model by the addition of two right handed neutrinos and three…

高能物理 - 唯象学 · 物理学 2020-02-19 Nayana Gautam , Mrinal Kumar Das

We derive constraints on parameters of the radiatively decaying Dark Matter (DM) particles, using XMM-Newton EPIC spectra of the Andromeda galaxy (M31). Using the observations of the outer (5'-13') parts of M31 we improve the existing…

天体物理学 · 物理学 2008-11-07 Alexey Boyarsky , Dmytro Iakubovskyi , Oleg Ruchayskiy , Vladimir Savchenko

The seesaw mechanism in models with extra dimensions is shown to be generically consistent with a broad range of Majorana masses. The resulting democracy of scales implies that the seesaw mechanism can naturally explain the smallness of…

高能物理 - 唯象学 · 物理学 2014-11-21 Alexander Kusenko , Fuminobu Takahashi , Tsutomu T. Yanagida

Neutrino masses and light (keV-GeV) sterile neutrinos can arise naturally via a modified, low energy seesaw mechanism if the right-handed neutrinos are charged under a new symmetry broken by a PeV scale vacuum expectation value, presumably…

高能物理 - 唯象学 · 物理学 2015-10-30 Bibhushan Shakya , Samuel B. Roland , James D. Wells

Sterile neutrinos may be one of the best Warm Dark Matter candidates we have today. Both lower and upper bounds on the mass of the sterile neutrino come from astronomical observations. We show that the proper inclusion of the neutrino…

天体物理学 · 物理学 2008-11-26 Steen H. Hansen , Julien Lesgourgues , Sergio Pastor , Joseph Silk

Recent measurements of PeV energy neutrinos at IceCube and a 3.5 keV X-ray line in the spectra of several galaxies are both tantalizing signatures of new physics. This paper shows that one or both of these observations can be explained…

高能物理 - 唯象学 · 物理学 2015-11-25 Samuel B. Roland , Bibhushan Shakya , James D. Wells
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