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相关论文: Mildly mixed coupled models vs. WMAP7 data

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The predictions of our previous analyses about possible low-mass (lower than 50 GeV) relic neutralinos are discussed in the light of the most recent results from WIMP direct detection experiments. It is proved that these light neutralinos…

高能物理 - 唯象学 · 物理学 2009-10-29 A. Bottino , F. Donato , N. Fornengo , S. Scopel

We consider two optimally mixed neutralino dark matter models, based on nonuniversal gaugino masses, which were recently proposed by us to achieve WMAP compatible relic density over a large part of the MSSM parameter space. We compare the…

高能物理 - 唯象学 · 物理学 2010-04-06 D. P. Roy

Recent DESI BAO measurements, combined with CMB data, reveal a tension within the $\Lambda$CDM model that leads to a discrepancy between cosmological and laboratory bounds on the summed neutrino mass. We show that a recoupled interacting…

宇宙学与河外天体物理 · 物理学 2026-05-19 Ravi Kumar Sharma , Maria Archidiacono , Julien Lesgourgues

We calculate the linear power spectrum for a range of mixed dark matter (MDM) models assuming a massive (few eV) boson, $\phi$, instead of a neutrino as the hot component. We consider both the case where the hot dark matter (HDM) particle…

天体物理学 · 物理学 2009-12-30 Georg B. Larsen , Jes Madsen

We discuss the physics potential of future tritium beta-decay experiments having a sensitivity to a neutrino mass ~\sqrt{|\Delta m^{2}_{23}|}~5x10^{-2} eV. The case of three-neutrino mixing is analised. A negative result of such an…

高能物理 - 唯象学 · 物理学 2008-11-26 S. M. Bilenky , M. D. Mateev , S. T. Petcov

In this paper, an electroweak model with massive neutrinos is proposed. The symmetry of the model is $SU(2)_L \times U(1)_Y \times U(1)_M$. Because of the mixing of neutrinos, the conversion of one lepton type to another is possible, but…

高能物理 - 唯象学 · 物理学 2007-05-23 Ning Wu

Dark matter and dark energy are usually assumed to couple only gravitationally. An extension to this picture is to model dark energy as a scalar field coupled directly to cold dark matter. This coupling leads to new physical effects, such…

宇宙学与河外天体物理 · 物理学 2015-06-22 Francesco Pace , Marco Baldi , Lauro Moscardini , David Bacon , Robert Crittenden

The predictions for the effective Majorana mass |<m>| in neutrinoless double-beta decay in the case of 3-neutrino mixing and massive Majorana neutrinos are reviewed. The physics potential of the experiments, searching for neutrinoless…

高能物理 - 唯象学 · 物理学 2007-05-23 S. Pascoli , S. T. Petcov

Dark matter (DM) and neutrinos are the two most compelling pieces of evidence of new physics beyond the Standard Model of Particle Physics but these are often treated as belonging to two different sectors. Yet DM-neutrino interactions are…

高能物理 - 唯象学 · 物理学 2017-05-12 Celine Boehm , Andres Olivares-Del Campo , Sergio Palomares-Ruiz , Silvia Pascoli

In this paper, we explore a scenario where the dark matter is a mixture of interacting and non interacting species. Assuming dark matter-photon interactions for the interacting species, we find that the suppression of the matter power…

宇宙学与河外天体物理 · 物理学 2020-02-05 Julia Stadler , Celine Bœhm , Olga Mena

An elegant model is proposed by extending the Standard Model using the $\Delta(27)\times Z_3 \times Z_{10}$ symmetry within the framework of the Type-I + Type-II seesaw mechanism. This model is particularly noteworthy for its ability to…

高能物理 - 唯象学 · 物理学 2025-03-26 Manash Dey , Subhankar Roy

Current measurements of the low and high redshift Universe are in tension if we restrict ourselves to the standard six parameter model of flat $\Lambda$CDM. This tension has two parts. First, the Planck satellite data suggest a higher…

宇宙学与河外天体物理 · 物理学 2014-02-10 Mark Wyman , Douglas H. Rudd , R. Ali Vanderveld , Wayne Hu

We present accurate predictions of the effective Majorana mass $|m_{\beta\beta}|$ in neutrinoless double-$\beta$ decay in the standard case of $3\nu$ mixing and in the case of 3+1 neutrino mixing indicated by the reactor, Gallium and LSND…

高能物理 - 唯象学 · 物理学 2015-09-02 C. Giunti , E. M. Zavanin

Couplings between light scalar dark matter (DM) and neutrinos induce a perturbation to the neutrino mass matrix. If the DM oscillation period is smaller than ten minutes (or equivalently, the DM particle is heavier than $0.69\times10^{-17}$…

高能物理 - 唯象学 · 物理学 2018-04-30 Jiajun Liao , Danny Marfatia , Kerry Whisnant

We briefly review some recent Cold Dark Matter (CDM) models. Our main focus are charge symmetric models of WIMPs which are not the standard SUSY LSP's (Lightest Supersymmetric Partners). We indicate which experiments are most sensitive to…

高能物理 - 唯象学 · 物理学 2009-10-29 Shmuel Nussinov

A simple and natural extension of the standard Lambda cold dark matter ($\Lambda$CDM) model is to allow relic neutrinos to have finite chemical potentials. We confront this $\Lambda$CDM$\xi$ model, a $\Lambda$CDM with neutrino mass $M_\nu$…

高能物理 - 唯象学 · 物理学 2025-09-03 Shek Yeung , Wangzheng Zhang , Ming-chung Chu

We calculate the linear evolution for a class of mixed dark matter models, where the hot component derives from the decay of a heavier particle (CntHDM models). These models differ from ordinary mixed models based on massive neutrinos (CHDM…

天体物理学 · 物理学 2009-09-25 E. Pierpaoli , S. Bonometto

$SU(2)_L$ triplet scalars appear in models motivated for the left-right symmetry, neutrino masses and dark matter (DM), etc.. If the triplets are the main decay products of the DM particle, and carry nonzero lepton numbers, they may decay…

高能物理 - 唯象学 · 物理学 2010-05-12 Wan-Lei Guo , Yue-Liang Wu , Yu-Feng Zhou

An explicit form of charged--lepton mass matrix, predicting $ m_\tau = 1776.80 $~MeV from the experimental values of $ m_e $ and $ m_\mu$ (in good agreement with the experimental figure $ m_\tau = 1777.05^{+0.29}_{-0.26}$ MeV), is applied…

高能物理 - 唯象学 · 物理学 2007-05-23 Wojciech Krolikowski

If the present or upcoming searches for neutrinoless double beta decay give a positive result, the Majorana nature of massive neutrinos will be established. From the determination of the value of the effective Majorana mass parameter |<m>|,…

高能物理 - 唯象学 · 物理学 2015-06-25 S. Pascoli , S. T. Petcov