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We study the effects of breaking S3 symmetry in the neutrino mass matrix for the masses and mixing matrix of neutrinos. At zeroth order the model gives degenerate neutrino masses and accommodates tribimaximal mixing. We introduce…

高能物理 - 唯象学 · 物理学 2012-02-16 S. Dev , Radha Raman Gautam , Lal Singh

The eigen mode of spin oscillations with $\omega\simeq \sqrt{58/35}\Delta$ is predicted to exist besides already known spin waves with $\omega \simeq\Delta /\sqrt{5}$ in the triplet superfluid neutron condensate in the inner core of neutron…

核理论 · 物理学 2011-08-09 L. B. Leinson

Our present work explores the possibility of neutrino mass generation through {\em Type-I see-saw} mechanism and provides an explanation of the baryon asymmetry of the Universe via thermal leptogenesis in the framework of $Z_3$-symmetric…

高能物理 - 唯象学 · 物理学 2020-09-08 Indrani Chakraborty , Himadri Roy

An experimentally verifiable Higgs-triplet model of neutrino masses from large extra dimensions was recently proposed. We extend it to accomodate a light sterile neutrino which also mixes with the three active neutrinos. A previously…

高能物理 - 唯象学 · 物理学 2009-10-31 Ernest Ma , G. Rajasekaran , Utpal Sarkar

The interplay between neutrino masses and the interactions of neutrinos with matter is discussed with an eye to extending the latter to include possible new interactions. This conjecture may resolve the conundrum posed by the present…

高能物理 - 唯象学 · 物理学 2007-05-23 Ernest Ma

The giant collective modes in asymmetric nuclear matter are investigated within a dynamic relaxation time approximation. We derive a coupled dispersion relation and show that two sources of coupling appear: (i) a coupling of isoscalar and…

核理论 · 物理学 2009-10-31 K. Morawetz , U. Fuhrmann , R. Walke

The separation method developed earlier by us [Nucl. Phys. {\bf A598} 390 (1996)] to calculate and analyze solutions of the BCS gap equation for $^1$S$_0$ pairing is extended and applied to $^3$P$_2$--$^3$F$_2$ pairing in pure neutron…

核理论 · 物理学 2008-11-26 V. V. Khodel , V. A. Khodel , J. W. Clark

We calculate the equation of state of neutron matter with realistic two- and three-nucleon interactions using quantum Monte Carlo techniques, and illustrate that the short-range three-neutron interaction determines the correlation between…

核理论 · 物理学 2012-03-15 S. Gandolfi , J. Carlson , Sanjay Reddy

For physically reasonable bulk and surface properties, quark matter has recently been found to coexist with nuclear matter inside neutron stars in a uniform background of electrons. The microstructure of this mixed phase starts out with a…

高能物理 - 唯象学 · 物理学 2009-09-25 H. HEISELBERG

We explore the possible formation of ordered phases in neutron star matter. In the framework of a quantum hadrodynamics model where neutrons, protons and Lambda hyperons interact via the exchange of mesons, we compare the energy of the…

核理论 · 物理学 2009-11-07 L. Mornas , J. P. Suarez Curieses , J. Diaz Alonso

We propose to determine the mass and the radius of a neutron star (NS) using three measurable mass-radius relationships, namely the ``apparent'' radius inferred from neutron star thermal emission, the gravitational redshift inferred from…

天体物理学 · 物理学 2008-11-26 C. M. Zhang , H. X. Yin , Y. Kojima , H. K. Chang , R. X. Xu , X. D. Li , B. Zhang , B. Kiziltan

Measurement of at least three independent parameters, for example, mass, radius and spin frequency, of a neutron star is probably the only way to understand the nature of its supranuclear core matter. Such a measurement is extremely…

高能天体物理现象 · 物理学 2015-05-14 Sudip Bhattacharyya

We study the dynamical evolution of a phase-transition-induced collapse neutron star to a hybrid star, which consists of a mixture of hadronic matter and strange quark matter. The collapse is triggered by a sudden change of equation of…

高能天体物理现象 · 物理学 2015-05-13 K. S. Cheng , T. Harko , Y. F. Huang , L. M. Lin , W. M. Suen , X. L. Tian

A triplet dark matter candidate from thermal leptogenesis is considered with building a model. The model is based on the standard two Higgs doublet model and seesaw mechanism with Higgs triplets. The parameters (couplings and masses) are…

高能物理 - 唯象学 · 物理学 2014-04-24 Jae Ho Heo , C. S. Kim

Matter at ultra-high densities finds a physical realization inside neutron stars. One key property is their maximum mass, which has far-reaching implications for astrophysics and the equation of state of ultra dense matter. In this work, we…

Recent studies invoke a unified description of different neutron star observables using metamodels, which parametrize the Equation of State (EoS) of neutron star matter close to nuclear saturation density in terms of few nuclear parameters.…

高能物理 - 唯象学 · 物理学 2026-03-26 José Luis Hernández , Cristina Manuel , Laura Tolos

Nuclear fission of several neutron-deficient actinides and pre-actinides from excitation energies around 11 MeV was studied at GSI Darmstadt by use of relativistic secondary beams. The characteristics of multimodal fission of nuclei around…

Neutrino energy losses through neutral weak currents in the triplet-spin superfluid neutron liquid are studied for the case of condensate involving several magnetic quantum numbers. Low-energy excitations of the multicomponent condensate in…

高能物理 - 唯象学 · 物理学 2011-10-25 L. B. Leinson

Nonuniform neutron-rich matter present in both core-collapse supernovae and neutron-star crusts is described in terms of a semiclassical model that reproduces nuclear-matter properties and includes long-range Coulomb interactions. The…

天体物理学 · 物理学 2009-11-10 C. J. Horowitz , M. A. Perez-Garcia , J. Carriere , D. K. Berry , J. Piekarewicz

We study the diffusive transport of neutrinos in a newly born neutron star to explore its sensitivity to dense matter properties. Energy and lepton number which are trapped during the catastrophic implosion diffuse out on the time scale of…

天体物理学 · 物理学 2007-05-23 S. Reddy , J. Pons , M. Prakash , J. M. Lattimer
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