搜索结果: 1-8 共查到“高能物理学 neutron”相关记录8条 . 查询时间(0.058 秒)
Formation of "Lightnings" in a Neutron Star Magnetosphere and the Nature of RRATs
neutron stars, pulsars, rotating radio transients.
2011/9/15
The connection between the radio emission from “lightnings” produced by the absorption of high-energy photons from the cosmic gamma-ray background in a neutron star magnetosphere and radio bursts from...
Neutron-gamma discrimination of CsI(Na) crystals for dark matter searches
Neutron-gamma discrimination CsI(Na) crystals dark matter
2011/4/7
Neutron-gamma discrimination of CsI(Na) crystals for dark matter searches 。
Motivated by an open question raised in recent times regarding the phase transition during the collapse of a neutron star to form a black hole and related stability issues, we have constructed charged...
Tkachenko modes in rotating neutron stars: the effect of compressibility and implications for pulsar timing noise
Tkachenko modes rotating neutron stars effect of compressibility implications pulsar timing noise
2010/12/21
Long wavelength oscillations (Tkachenko waves) of the triangular lattice of quantized vortices in super uid neutron stars have been suggested as one of the possible explanations for the timing noise o...
Evolutions of Magnetized and Rotating Neutron Stars
Rotating Neutron Stars Evolutions of Magnetized
2010/3/17
We study the evolution of magnetized and rigidly rotating neutron stars within a fully general relativistic implementation of ideal magnetohydrodynamics with no assumed symmetries in three spatial dim...
The Density-Dependent Correlations among Observables in Nuclear Matter and Hyperon-Rich Neutron Stars
Nuclear Matter Hyperon-Rich Neutron Stars Density-Dependent
2009/9/4
The conserving σ-ω-ρ mean-field approximation with nonlinear interactions of hadrons has been applied to examine properties of nuclear matter and hyperonic neutron stars. The nonlinear interactions th...
Antikaon condensation in neutron star matter with strong magnetic fields
quark-meson coupling model antikaon condensation magnetic fields
2009/8/17
We study the influence of strong magnetic fields on antikaon condensation in neutron star matter using the quark-meson coupling (QMC) model. The QMC model describes a nuclear many-body system as nonov...
Hadron-quark phase transition in neutron stars
hadron-quark phase transition equation of state neutron stars
2009/8/14
We study the hadron-quark phase transition in the interior of neutron stars. The relativistic mean field (RMF) theory is adopted to describe the hadronic matter phase, while the Nambu-Jona-Lasinio (NJ...