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相关论文: Neutron rich matter in heaven and on Earth

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Neutron stars -- compact objects with masses similar to that of our Sun but radii comparable to the size of a city -- contain the densest form of matter in the universe that can be probed in terrestrial laboratories as well as in earth- and…

核理论 · 物理学 2022-10-06 J. Piekarewicz

Neutron stars are some of the densest manifestations of massive objects in the universe. They are ideal astrophysical laboratories for testing theories of dense matter physics and provide connections among nuclear physics, particle physics…

天体物理学 · 物理学 2011-05-05 J. M. Lattimer , M. Prakash

We explore the unique and fascinating structure of neutron stars. Although neutron stars are of interest in many areas of Physics, our aim is to provide an intellectual bridge between Nuclear Physics and Astrophysics. We argue against the…

核理论 · 物理学 2015-06-18 J. Piekarewicz

One of the most intringuing questions about neutron stars concerns their maximum mass. The answer is intimately related to the properties of matter at densities far beyond that found in heavy atomic nuclei. The current view on the internal…

高能天体物理现象 · 物理学 2013-11-19 N. Chamel , P. Haensel , J. L. Zdunik , A. F. Fantina

With central densities way above the density of atomic nuclei, neutron stars contain matter in one of the densest forms found in the universe. Depending of the density reached in the cores of neutron stars, they may contain stable phases of…

天体物理学 · 物理学 2010-12-06 Fridolin Weber , Matthew Meixner , Rodrigo P. Negreiros , Manuel Malheiro

In the standard picture of the crust of a neutron star, matter there is simple: a body-centered-cubic (bcc) lattice of nuclei immersed in an essentially uniform electron gas. We show that at densities above that for neutron drip…

核理论 · 物理学 2015-06-17 D. Kobyakov , C. J. Pethick

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

A neutron star is pictured as a gigantic nucleus overwhelmed by the number of neutrons, unlike real atomic nuclei, that have a similar number of neutrons and protons. Is this true? What if we could find, or create nuclei without protons?…

核实验 · 物理学 2021-06-02 F. Miguel Marqués

Neutron matter is an intriguing nuclear system with multiple connections to other areas of physics. Considerable progress has been made over the last two decades in exploring the properties of pure neutron fluids. Here we begin by reviewing…

核理论 · 物理学 2015-10-27 Stefano Gandolfi , Alexandros Gezerlis , J. Carlson

Neutron stars are highly compact astrophysical objects and therefore of utmost relevance to learn about theories of gravity. Whereas the proper equation of state of the nuclear matter inside neutron stars is not yet known, and a wide range…

广义相对论与量子宇宙学 · 物理学 2022-04-28 Jutta Kunz

A short introduction is given to astrophysics of neutron stars and to physics of dense matter in neutron stars. Observed properties of astrophysical objects containing neutron stars are discussed. Current scenarios regarding formation and…

天体物理学 · 物理学 2007-05-23 Marek Kutschera

Neutron Stars (NSs) are compact stellar objects that are stable solutions in General Relativity. Their internal structure is usually described using an equation of state that involves the presence of ordinary matter and its interactions.…

高能天体物理现象 · 物理学 2020-12-18 M. Ángeles Pérez-García , J. Silk

Because of the tremendous densities that exist in the cores of neutron stars, a significant fraction of the matter in the cores of such stars is likely to exist in the form of hyperons. Depending on spin frequency, the hyperon content…

天体物理学 · 物理学 2007-05-23 Fridolin Weber , Philip Rosenfield

Recent observations of neutron star masses close to the maximum predicted by nucleonic equations of state begin to challenge our understanding of dense matter in neutron stars, and constrain the possible presence of quark matter in their…

核理论 · 物理学 2008-11-26 Gordon Baym

What is the size of the atomic nucleus? This deceivably simple question is difficult to answer. While the electric charge distributions in atomic nuclei were measured accurately already half a century ago, our knowledge of the distribution…

Even the elusive neutrinos are trapped in matter, albeit transiently, in several astrophysical circumstances. Their interactions with the ambient matter not only reveal the properties of such exotic matter itself, but also shed light on the…

天体物理学 · 物理学 2009-11-06 M. Prakash , J. M. Lattimer , R. F. Sawyer , R. R. Volkas

Formed in the aftermath of gravitational core-collapse supernova explosions, neutron stars are unique cosmic laboratories for probing the properties of matter under extreme conditions that cannot be reproduced in terrestrial laboratories.…

核理论 · 物理学 2019-03-06 David Blaschke , Nicolas Chamel

Neutron stars contain matter in one of the densest forms found in the Universe. This feature, together with the unprecedented progress in observational astrophysics, makes such stars superb astrophysical laboratories for a broad range of…

天体物理学 · 物理学 2007-05-23 F. Weber , R. Negreiros , P. Rosenfield

Neutron stars are one of the most extreme objects in the universe, with densities that can exceed those of atomic nuclei and gravitational fields that are among the strongest known. Theoretical and observational research on neutron stars…

高能天体物理现象 · 物理学 2023-03-16 J. Alfredo Collazos

Neutron stars are unique cosmic laboratories for the exploration of matter under extreme conditions of density and neutron-proton asymmetry. Due to their enormous dynamic range, neutron stars display a myriad of exotic states of matter that…

核理论 · 物理学 2018-05-18 J. Piekarewicz
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