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From the observed results, we deduced that the mass of the neutrino is about 10^(-1) eV and the mass of the fourth stable elementary particle (delta) is about 10^(0) eV. While neutrino is related to electro-weak field, the fourth stable…

综合物理 · 物理学 2016-12-26 Xiaodong Huang , Wuliang Huang

From the observed results of the space distribution of quasars we deduced that neutrino mass is about10^(-1) eV. The fourth stable elementary particle (delta particle) with mass about 10^(0) eV can help explain the energy resource mechanism…

综合物理 · 物理学 2024-01-30 Xiaodong Huang , Wuliang Huang

High energy particles are produced by the annihilation of dark matter particles in our galaxy. These are presently searched for using balloon-borne antiproton and positron detectors and large area, deep underground neutrino telescopes. Dark…

高能物理 - 唯象学 · 物理学 2016-09-01 F. Halzen , J. E Jacobsen

We extend mass scale sequence to a mass tree. From mass tree, the evolution of the universe is described by three stages: chaos, inflation and expansion. The first two stages have c mutations and the inflation appears as a step by step…

综合物理 · 物理学 2020-05-06 Wuliang Huang , Xiaodong Huang

Despite direct observations favoring a low mass density, a critical density universe with a neutrino component of dark matter provides the best existing model to explain the observed structure of the universe over more than three orders of…

天体物理学 · 物理学 2009-10-31 David O. Caldwell

Solar, atmospheric and reactor neutrino experiments established that neutrinos are massive. It is quite natural then to consider neutrinos as candidate particles for explaining the dark matter in halos around galaxies. We study the…

高能物理 - 唯象学 · 物理学 2015-06-04 A. Nicolaidis

All presently known stellar-dynamical constraints on the size and mass of the supermassive compact dark object at the Galactic center are consistent with a ball of self-gravitating, nearly non-interacting, degenerate fermions with mass…

天体物理学 · 物理学 2007-05-23 Neven Bilic , Gary B. Tupper , Raoul D. Viollier

There are strong indications for neutrino masses and mixings in the data on solar neutrinos as well as in the observed deficit of muon neutrinos from the atmosphere. The COBE data and other analysis of the large scale structure in the…

高能物理 - 唯象学 · 物理学 2007-05-23 R. N. Mohapatra

A new era in particle physics is being spurred on by new data from the Large Hadron Collider. Non-vanishing neutrino masses represent firm observational evidence of new physics beyond the Standard Model. An extension of the latter, based on…

高能物理 - 唯象学 · 物理学 2015-06-05 S. Khalil , S. Moretti

We show that the neutrino mass, the dark matter and the dark energy can be explained in a unified framework, postulating a new invisible Born-Infeld field, which we name "non-linear dark photon", undergoing a meV-scale dynamical…

高能物理 - 唯象学 · 物理学 2022-08-09 Andrea Addazi , Salvatore Capozziello , Qingyu Gan , Antonino Marcianò

Even though neutrinos and antineutrinos are everywhere in the Universe, their critical importance might be overlooked, especially because that at least one species of neutrinos has the mass 0.058 eV, far larger than the cosmic…

高能物理 - 唯象学 · 物理学 2016-01-14 W-Y. Pauchy Hwang

The energy scale of Dark Energy, $\sim 2 \times 10^{-3}$ eV, is a long way off compared to all known fundamental scales - except for the neutrino masses. If Dark Energy is dynamical and couples to neutrinos, this is no longer a coincidence.…

宇宙学与河外天体物理 · 物理学 2016-03-23 Youness Ayaita , Marco Baldi , Florian Führer , Ewald Puchwein , Christof Wetterich

We propose a simple extension of the standard model by adding a fourth generation vector-like lepton doublet and show that if the fourth neutrino is a massive pseudo-Dirac fermion with mass in the few hundred GeV range and mass splitting of…

高能物理 - 唯象学 · 物理学 2015-06-12 Chiara Arina , Rabindra N. Mohapatra , Narendra Sahu

We study the degeneracies between neutrino mass and dark energy as they manifest themselves in cosmological observations. In contradiction to a popular formula in the literature, the suppression of the matter power spectrum caused by…

天体物理学 · 物理学 2008-11-26 Angeliki Kiakotou , Oystein Elgaroy , Ofer Lahav

There is a puzzling contradiction: direct observations favor a low-mass density universe, but the only model which fits universe structure over more than three orders of magnitude in distance scale has a mix of hot (neutrino) and cold dark…

高能物理 - 唯象学 · 物理学 2007-05-23 David O. Caldwell

We study a simple extension of the standard model to simultaneously explain neutrino masses, dark matter and the matter-antimatter asymmetry of the Universe. In our model, the baryon asymmetry is achieved by the leptogenesis mechanism,…

高能物理 - 唯象学 · 物理学 2010-03-26 Chuan-Hung Chen , Chao-Qiang Geng , Dmitry V. Zhuridov

More than sixty years ago Zwicky made the case that the great clusters of galaxies are held together by the gravitational force of unseen (dark) matter. Today, the case is stronger and more precise: Dark, nonbaryonic matter accounts for 30%…

天体物理学 · 物理学 2016-11-23 Michael S. Turner

The Standard Model (SM) is inadequate to explain the origin of tiny neutrino masses, the dark matter (DM) relic abundance and also the baryon asymmetry of the Universe. In this work to address all the three puzzles, we extend the SM by a…

高能物理 - 唯象学 · 物理学 2017-12-19 Anirban Biswas , Sandhya Choubey , Sarif Khan

We propose a model to explain tiny masses of neutrinos with the lepton number conservation, where neither too heavy particles beyond the TeV-scale nor tiny coupling constants are required. Assignments of conserving lepton numbers to new…

高能物理 - 唯象学 · 物理学 2017-11-29 Shinya Kanemura , Kodai Sakurai , Hiroaki Sugiyama

We propose a new scenario of incorporating neutrino masses in models of TeV scale gravity and large extra dimensions, which can explain the dark energy problem through formation of neutrino condensates. The smallness of the neutrino masses…

高能物理 - 唯象学 · 物理学 2022-05-03 Ujjal Kumar Dey , Utpal Sarkar
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