搜索结果: 1-8 共查到“理学 dense matter”相关记录8条 . 查询时间(0.135 秒)
Symmetry energy of dense matter in holographic QCD
Symmetry energy dense matter holographic QCD
2010/12/24
We study the nuclear symmetry energy of dense matter using holographic QCD. To this end, we consider two flavor branes with equal quark masses in a D4/D6/D6 model. We find that at high density the sym...
Heavy mesons in dense matter
Heavy mesons dense matter
2010/12/29
Charmed mesons in dense matter are studied within a unitary coupled-channel approach which takes into account Pauli-blocking effects and meson self-energies in a self-consistent manner. We obtain the ...
Symmetry energy of dense matter in holographic QCD
Symmetry energy of dense matter holographic QCD
2011/1/7
We study the nuclear symmetry energy of dense matter using holographic QCD. To this end, we
consider two flavor branes with equal quark masses in a D4/D6/D6 model. We find that at high
density the s...
Rapid Cooling of the Neutron Star in Cassiopeia A Triggered by Neutron Superfluidity in Dense Matter
Rapid Cooling of the Neutron Star Cassiopeia Neutron Superfluidity
2011/1/10
We propose that the recently observed cooling of the neutron star in Cassiopeia A is due to
enhanced neutrino emission from the onset of the breaking and formation of neutron Cooper pairs
in the 3P2...
Heavy mesons in dense matter
charm meson dynamically generated resonance mesic nuclei heavy-quark symmetry
2011/1/7
Charmed mesons in dense matter are studied within a unitary coupled-channel approach which takes into account Pauli-blocking effects and meson self-energies in a self-consistent manner.We obtain the o...
Heavy mesons in dense matter
charm meson dynamically generated resonance mesic nuclei heavy-quark symmetry
2011/1/6
Charmed mesons in dense matter are studied within a unitary coupled-channel approach which takes into account Pauli-blocking effects and meson self-energies in a self-consistent manner.We obtain the o...
Internal heating and thermal emission from old neutron stars：constraints on dense-matter and gravitational physics
old neutron stars gravitational physics dense-matter
2009/6/25
Internal heating and thermal emission from old neutron stars：constraints on dense-matter and gravitational physics。
THE ORIGIN OF ROTATION, DENSE MATTER PHYSICS AND ALL THAT: A TRIBUTE TO PAVLE SAVIC
PAVLE SAVIC DENSE MATTER PHYSICS ORIGIN OF ROTATION
2009/4/16
THE ORIGIN OF ROTATION, DENSE MATTER PHYSICS AND ALL THAT: A TRIBUTE TO PAVLE SAVIC。