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We study a model of neutrino and dark matter within the framework of a minimal extended seesaw. This framework is based on $A_4$ flavor symmetry along with the discrete $Z_4$ symmetry to stabilize the dark matter and construct desired mass…

高能物理 - 唯象学 · 物理学 2020-04-22 Pritam Das , Mrinal Kumar Das , Najimuddin Khan

Massive neutrinos suppress the growth of cosmic structure on small, non-linear, scales. It is thus often proposed that using statistics beyond the power spectrum can tighten constraints on the neutrino mass by extracting additional…

宇宙学与河外天体物理 · 物理学 2022-06-16 Adrian E. Bayer , Arka Banerjee , Uros Seljak

Working in the context of a Lorentz-violating extension of the standard model we show that estimates of Lorentz symmetry violation extracted from ultra-high energy cosmic rays beyond the Greisen-Kuzmin-Zatsepin (GZK) cutoff allow for…

广义相对论与量子宇宙学 · 物理学 2008-11-26 O. Bertolami , C. S. Carvalho

We examine the prospects for determining the neutrino mixing matrix and for observing CP and T violation in neutrino oscillations in four-neutrino models. We focus on a general class of four-neutrino models with two pairs of nearly…

高能物理 - 唯象学 · 物理学 2009-09-15 V. Barger , Yuan-Ben Dai , K. Whisnant , Bing-Lin Young

Extending the Standard Model with right-handed neutrinos provides a minimal explanation for both light neutrino masses (through the type-I seesaw mechanism) and the baryon asymmetry of our universe (through leptogenesis). We map here for…

高能物理 - 唯象学 · 物理学 2023-05-12 Yannis Georis

We determine the restrictions imposed by primordial nucleosynthesis upon a heavy tau neutrino, in the presence of nu-tau annihilations into Majorons, as expected in a wide class of particle physics models of neutrino mass. We determine the…

高能物理 - 唯象学 · 物理学 2009-09-17 A. D. Dolgov , S. Pastor , J. C. Romao , J. W. F. Valle

The ages and masses of neutron stars (NSs) are two fundamental threads that make pulsars accessible to other sub-disciplines of astronomy and physics. A realistic and accurate determination of these two derived parameters play an important…

星系天体物理 · 物理学 2015-05-27 Bulent Kiziltan

We consider a model based on $A_4$ symmetry to explain the phenomenon of neutrino mixing. The spontaneous symmetry breaking of $A_4$ symmetry leads to a co-bimaximal mixing matrix at leading order. We consider the effect of higher order…

高能物理 - 唯象学 · 物理学 2017-04-05 Sruthilaya M. , R. Mohanta

Neutrino masses and mixings are analyzed in terms of left-handed fields and a 6x6 complex symmetric mass matrix whose singular values are the neutrino masses. An angle x_nu characterizes the kind of the neutrinos, with x_nu = 0 for Dirac…

高能物理 - 唯象学 · 物理学 2007-05-23 Kevin Cahill

Weak gravitational lensing of background galaxies by intervening matter directly probes the mass distribution in the universe. This distribution, and its evolution at late times, is sensitive to both the dark energy, a negative pressure…

天体物理学 · 物理学 2009-11-07 Kevork Abazajian , Scott Dodelson

We analyze the effect of a variation of the strange nucleon matrix element $\langle N| m_s \bar{s}s|N\rangle$ on the abundances of the light elements produced in the Big Bang. For that, we vary the nucleon mass in the leading eight…

高能物理 - 唯象学 · 物理学 2025-02-24 Ulf-G. Meißner , Bernard Metsch , Helen Meyer

The weak lensing (WL) distortions of distant galaxy images are sensitive to neutrino masses by probing the suppression effect on clustering strengths of total matter in large-scale structure. We use the latest measurement of WL…

天体物理学 · 物理学 2010-04-21 Kiyotomo Ichiki , Masahiro Takada , Tomo Takahashi

Recently we presented a simple method for determining the correlated uncertainties of the light element abundances expected from big bang nucleosynthesis, which avoids the need for lengthy Monte Carlo simulations. We now extend this…

高能物理 - 唯象学 · 物理学 2008-11-26 E. Lisi , Subir Sarkar , F. L. Villante

Model-independent mass limits assess the robustness of current cosmological measurements of the neutrino mass scale. Consistency between high-multipole and low-multiple Cosmic Microwave Background observations measuring such scale further…

宇宙学与河外天体物理 · 物理学 2023-10-12 Eleonora Di Valentino , Stefano Gariazzo , William Giarè , Olga Mena

We discuss consequences of assuming that the (Majorana) neutrino mass matrix $M_\nu$ and the charged lepton mass matrix $M_l$ satisfy, $S_\nu^T M_\nu S_\nu=-M_\nu~,T_l^\dagger M_lM_l^\dagger T_l=M_lM_l^\dagger$ with respect to some discrete…

高能物理 - 唯象学 · 物理学 2016-08-31 Anjan S Joshipura , Newton Nath

We investigate a radiative seesaw model with two leptoquarks under non-holomorphic modular $A_4$ symmetry. The leptons and quarks belong to non-trivial representations of the modular $A_4$ and the structures of their mass matrices are…

高能物理 - 唯象学 · 物理学 2025-05-14 Takaaki Nomura , Hiroshi Okada , Xing-Yu Wang

A search for heavy neutral lepton ($N$) production in $K^+\to e^+N$ decays using the data sample collected by the NA62 experiment at CERN in 2017--2018 is reported. Upper limits of the extended neutrino mixing matrix element $|U_{e4}|^2$…

高能物理 - 实验 · 物理学 2020-07-08 NA62 collaboration

We present the results of a search for new particles with long lifetime that decay to a Z boson. A long-lived parent of the Z is predicted by several models in addition to being an experimentally clean channel. We vertex dimuons with…

高能物理 - 实验 · 物理学 2010-04-22 Adam L. Scott , representing the CDF Collaboration

We suggest a low-scale model based on $A_4\times Z_4 \times Z_2$ symmetry and a global lepton number $U(1)_L$ symmetry capable of generating the current neutrino data. The neutrino mass smallness is reproduced by the linear seesaw…

高能物理 - 唯象学 · 物理学 2023-02-08 V. V. Vien , H. N. Long

With the accumulation of many years of solar and atmospheric neutrino oscillation data, the approximate form of the 3 times 3 neutrino mixing matrix is now known. What is not known is the (presumably Majorana) neutrino mass matrix M_{nu}…

高能物理 - 唯象学 · 物理学 2007-05-23 Ernest Ma
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