This book is a comprehensive collection of thirteen reviews of many aspects of neutron stars motivated by the NewCompStar network, funded through the European Cooperation in Science and Technology, which between 2013 and 2017 encouraged the interdisciplinary (astrophysics, gravitational physics and nuclear...
The death of that star is the birth of a neutron star: 那个星体的死亡,成了一个中子星的诞生: one of the densest known objects in the universe, 中子星是全宇宙最高密度的已知物体之一, and a laboratory for the strange physics of supercondensed matter. 它也是超级压缩物质的奇异物理实验室。 But...
This new neutrino physics also may have heavy important for nuclear physics and astrophysics. This is because neutrinos and their interactions with nuclei and nucleons are instrumental in setting the conditions which determine the synthesis of the light elements in the early universe and possibly the...
The physics of neutron stars is a remarkable combination of Einstein’s theory of general relativity and nuclear physics. Their interiors harbour extreme matter that cannot be probed in the laboratory. At such high densities and pressures, their cores may consist predominantly of exotic matter, such...
Neutron Star Interiors and the Equation of State of Superdense Matter There has been much recent progress in our understanding of quark matter, culminating in the discovery that if such matter exists in the cores of neutron s... F Weber,R Negreiros,P Rosenfield - American Institute of Physics...
A NICER View: Astrophysics and Exploration from the International Space Station (NICER) mission aims to answer longstanding questions about the physics and astrophysics of neutron stars, with a telescope on the International Space Station designed to investigate their X-ray emissions and time their pul...
- Conference on 40 Years of Pulsars 被引量: 0发表: 2008年 The Birth of Neutron Stars and Black Holes We report here on recent progress in understanding the birth conditions of neutron stars and the way how supernovae explode. More sophisticated numerical m... Burrows,Adam - 《Physics ...
Integral observations of polarization: From the Crab pulsar to Cygnus X-1 In complement to spectro-imaging observations, γ-ray polarimetry provides a unique insight into the geometry and magnetic configuration of compact γ-ray sources, such as neutron stars or black holes. Due to the unprecedente...
(the photo-thermal quantum-evaporation and bond-breaking energy and the dark-cold quantum-condensation and bond-forming energy) and the cosmic subquantum etheric-leveled electromagnetic streams-intercutting and entangling web, to develop a potentially omnipotent theory of new astro-particle physics. ...
For most of their existence, stars are fuelled by the fusion of hydrogen into helium. Fusion proceeds via two processes that are well understood theoretically: the proton–proton (pp) chain and the carbon–nitrogen–oxygen (CNO) cycle1,2. Neutrinos that