✦ LIBER ✦

The final phase of inspiral of neutron stars: Realistic equations of state

✍ Scribed by D. Gondek-Rosińska; M. Bejger; T. Bulik; E. Gourgoulhon; Paweł Haensel; F. Limousin; K. Taniguchi; L. Zdunik

Book ID: 108065912
Publisher: Elsevier Science
Year: 2007
Tongue: English
Weight: 227 KB
Volume: 39
Category: Article
ISSN: 0273-1177
DOI: 10.1016/j.asr.2006.09.021

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

Equilibrium configurations of strongly m

Equilibrium configurations of strongly magnetized neutron stars with realistic equations of state

✍ Kenta Kiuchi; Kei Kotake 📂 Article 📅 2008 🏛 John Wiley and Sons 🌐 English ⚖ 371 KB

Quark stars with ‘realistic’ equations o

Quark stars with ‘realistic’ equations of state

✍ FECHNER, W. B.; JOSS, P. C. 📂 Article 📅 1978 🏛 Nature Publishing Group 🌐 English ⚖ 284 KB

Equation of state, neutron stars and exo

Equation of state, neutron stars and exotic phases

✍ James M. Lattimer; Madappa Prakash 📂 Article 📅 2006 🏛 Elsevier Science 🌐 English ⚖ 580 KB

The role of the equation of state in the structure of neutron stars is summarized. At densities beyond a few times the normal nuclear saturation density, the neutron-proton-electron sea can be supplemented with more exotic matter, usually involving strangeness, such as hyperons, kaon or pion condens

General-relativistic decompression of bi

General-relativistic decompression of binary neutron stars during dynamic inspiral

✍ Miller, Mark 📂 Article 📅 2007 🏛 The American Physical Society 🌐 English ⚖ 324 KB

The equation of state for neutron stars

✍ F. Ferrini 📂 Article 📅 1975 🏛 Springer Netherlands 🌐 English ⚖ 549 KB

Can magnetic fields be detected during t

Can magnetic fields be detected during the inspiral of binary neutron stars?

✍ Bruno Giacomazzo; Luciano Rezzolla; Luca Baiotti 📂 Article 📅 2009 🏛 John Wiley and Sons 🌐 English ⚖ 563 KB