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相关论文: Z-lineshape versus 4th generation masses

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We consider the neutrino sector of a Standard Model with four generations. While the three light neutrinos can obtain their masses from a variety of mechanisms with or without new neutral fermions, fourth-generation neutrinos need at least…

高能物理 - 唯象学 · 物理学 2015-06-04 Alberto Aparici , Juan Herrero-García , Nuria Rius , Arcadi Santamaria

We continue our previous determination of the masses of the sequential fourth generation quarks in an extension of the Standard Model, and predict the mass $m_4$ ($m_L$) of the fourth generation neutrino $\nu_4$ (charged lepton $L$) by…

高能物理 - 唯象学 · 物理学 2024-12-20 Hsiang-nan Li

We investigate the possibility of a fourth sequential generation in the lepton sector. Assuming neutrinos to be Majorana particles and starting from a recent - albeit weak - evidence for a non-zero admixture of a fourth generation neutrino…

高能物理 - 唯象学 · 物理学 2012-05-03 Alexander Lenz , Heinrich Päs , Dario Schalla

We present new constraints on the mass $m_{\nu_\tau}$ of the tau neutrino and its mixing with a fourth generation neutrino. From an analysis of the partial widths of tau lepton decays we obtain the following bounds at the 90% confidence…

高能物理 - 唯象学 · 物理学 2007-05-23 John Swain , Lucas Taylor

The case for small neutrino mass differences from atmospheric and solar neutrino oscillation experiments has become compelling, but leaves the overall neutrino mass scale m_nu undetermined. The most restrictive limit of m_nu < 0.8 eV arises…

天体物理学 · 物理学 2009-11-07 G. G. Raffelt

Current mass limits for fourth generation sequential neutrinos come from dark matter experiments assuming $\rho_{DM}=0.2-0.8$ g/ cm$^3$. We show that the latest results from the CDMS II experiment exclude Dirac neutrinos with masses below…

高能物理 - 实验 · 物理学 2007-05-23 Gray Rybka , Peter Fisher

We overview the constraints on the 4th-generation neutrino dark matter candidate and investigate a possible way to make it a viable dark matter candidate. Given the LEP constraints tell us that the 4th-generation neutrino has to be rather…

高能物理 - 唯象学 · 物理学 2011-09-20 Hye-Sung Lee , Zuowei Liu , Amarjit Soni

In this talk we explore the possibility that the smallness of the observed neutrino masses is naturally understood in a modified version of the standard model with N extra generations of fermions and N right-handed neutrinos, in which light…

高能物理 - 唯象学 · 物理学 2014-10-15 A. Aparici , J. Herrero-Garcia , N. Rius , A. Santamaria

The 4th generation of fermions predicted by the phenomenology of heterotic string models can possess new strictly conserved charge, which leads, in particular, to the hypothesis of the existence of the 4th generation massive stable…

天体物理学 · 物理学 2009-10-31 D. Fargion , Yu. A. Golubkov , M. Yu. Khlopov , R. V. Konoplich , R. Mignani

We study the effect of neutrino degeneracy on primordial nucleosynthesis in a universe in which the cosmological scale factor evolves linearly with time. The degeneracy parameter of electron type neutrinos ($\xi_e$) determines the $n/p$…

宇宙学与河外天体物理 · 物理学 2015-06-02 Parminder Singh , Daksh Lohiya

It is supposed that the electron neutrino mass is related to the structures and masses of the $W^\pm$ and $Z^0$ bosons. Using a composite model of fermions (described elsewhere), it is shown that the massless neutrino is not consistent with…

综合物理 · 物理学 2007-05-23 V. N. Yershov

We explore the possible implications that new families, that are being searched for at the LHC, would have on neutrino masses. In particular, we have explored the possibility that the smallness of the observed neutrino masses is naturally…

高能物理 - 唯象学 · 物理学 2011-10-05 A. Aparici , J. Herrero-Garcia , N. Rius , A. Santamaria

Our knowledge of the neutrino sector of the Standard Model has recently undergone a revolution. Deficits of the atmospheric muon neutrino flux and the solar electron neutrino flux compared to their predicted values can be understood in…

高能物理 - 唯象学 · 物理学 2009-10-31 V. Barger

Four zero neutrino Yukawa textures in a specified weak basis, combined with $\mu\tau$ symmetry and type-I seesaw, yield a highly constrained and predictive scheme. Two alternately viable $3\times3$ light neutrino Majorana mass matrices…

高能物理 - 唯象学 · 物理学 2015-05-27 Biswajit Adhikary , Ambar Ghosal , Probir Roy

We reconsider the possibility that Majorana masses for the three known neutrinos are generated radiatively by the presence of a fourth generation and one right-handed neutrino with Yukawa couplings and a Majorana mass term. We find that the…

高能物理 - 唯象学 · 物理学 2011-08-01 Alberto Aparici , Juan Herrero-García , Nuria Rius , Arcadi Santamaria

We revisit the current experimental bounds on fourth-generation Majorana neutrino masses, including the effects of right handed neutrinos. Current bounds from LEPII are significantly altered by a global analysis. We show that the current…

高能物理 - 唯象学 · 物理学 2011-01-17 Linda M. Carpenter , Arvind Rajaraman

We consider the bounds for the values of higgs mass $m_H$ and the mass of the extra quarks and leptons $m_{extra}$ derived from the stability of electroweak vacuum and from the absence of Landau pole in Higgs potential. We find that in the…

高能物理 - 唯象学 · 物理学 2007-05-23 V. A. Novikov

With the recent experimental advance in our precise knowledge of the neutrino oscillation parameters, the correct form of the 3 X 3 neutrino mass matrix is now approximately known. I discuss how this may be obtained from symmetry…

高能物理 - 唯象学 · 物理学 2007-05-23 Ernest Ma

Results from several recent experiments provide inderect evidences in the favor of existence of a 4th generation neutrino. Such a neutrino of mass about 50 GeV is compatible with current physical and astrophysical constraints and well…

高能物理 - 唯象学 · 物理学 2009-11-07 K. Belotsky , D. Fargion , M. Khlopov , R. Konoplich , K. Shibaev

A range of experimental results point to the existence of a massive neutrino. The recent high precision measurements of the cosmic microwave background and the large scale surveys of galaxies can be used to place an upper bound on this…

天体物理学 · 物理学 2009-06-12 C. Zunckel , P. G Ferreira
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