We start with a brief introduction to the historical background in the early pioneering days when the first neutron star thermal evolution calculations predicted the presence of neutron stars hot enough to be observable. We then report on the first detection of neutron star temperatures by ROSAT X...
The surface of a neutron star is around 600,000 degrees C (around 1 million degrees Fahrenheit).What is the Sun? The Sun is the center of the solar system. At the center of the solar system is a star—the Sun. While it shares many characteristics with other stars in the galaxy, it...
2.This article studies neutron star matter atfinite temperaturein the framework of the relativistic mean field theory.本文采用先进的计算技术克服了传统计算方法中处理有限温下费米-狄拉克函数的无穷展开的困难,在相对论平均场(RMFT)框架内,研究了有限温下中子星物质的四个相关问题。
We then consider a model for the spectrum of the X-ray emission from the disk, parameterized by the mass accretion rate, the color temperature and the rotation rate of the neutron star. We derive constraints on these parameters for the X-ray source Cygnus X-2 using the estimates of the ...
2. the effect of a strong toroidal component We continue the study of the effects of a strong magnetic field on the temperature distribution in the crust of a magnetized neutron star (NS) and its impact on the observable surface temperature. Extending the approach initiated in Gepp... U ...
Using these methods thermal Nyquist noise is reduced such that the antenna effective temperature is reduced to a few microdegrees. A world-wide array of detectors should now allow any gravitational collapse which gives rise to the birth of a neutron star or black hole to be detected anywhere ...
The various effective interactions'(including DDME1,TW99,NL2,TM1,TM2,GL85 and GL97) influence on the constitute,equation of state and mass of neutron star are studied in the framework of relativistic mean field theory considering the interacting nucleons,hyperons and mesons system at finite tem...
Understanding how different physical processes can shape the probability distribution function (PDF) of surface temperature, in particular the tails of the... A Berg,BR Lintner,KL Findell,... - 《Journal of Climate》 被引量: 68发表: 2014年 Temperature distribution in magnetized neutron star crust...
S-process neutron capture is slower than beta-decay atstellar temperaturesgenerated by exothermic nuclear fusion reactions and is unable to bridge the gap between the long-lived bismuth isotopes (82208Bi,82209Bi, and82211Bi) to long-lived thoriumisotopes (90230Th and90232Th).9Most of the neutro...
1) finite-temperature neutron star 有限温度中子星2) finite temperature 有限温度 1. A two-dimensional dark energy star model at finite temperature; 有限温度下的二维暗能量星模型 2. The energy and thermal effects of mesoscopic capacitance coupling LC circuit at finite temperature; 介观电容耦合LC...