Baryonic properties of neutron stars within pseudo-complex General Relativity

2014 ◽  
Vol 335 (6-7) ◽  
pp. 745-750 ◽  
Author(s):  
I. Rodríguez ◽  
P. O. Hess ◽  
S. Schramm ◽  
W. Greiner
Keyword(s):  
General Relativity ◽  
Neutron Stars ◽  
Complex General Relativity

Pseudo-complex General Relativity and neutron stars

2014 ◽  
Vol 335 (6-7) ◽  
pp. 679-684 ◽  
Author(s):  
P. O. Hess ◽  
I. Rodríguez ◽  
W. Greiner
Keyword(s):  
General Relativity ◽  
Neutron Stars ◽  
Complex General Relativity

Neutron stars within pseudo-complex general relativity

2014 ◽  
Vol 41 (10) ◽  
pp. 105201 ◽  
Author(s):  
Isaac Rodríguez ◽  
Peter O Hess ◽  
Stefan Schramm ◽  
Walter Greiner
Keyword(s):  
General Relativity ◽  
Neutron Stars ◽  
Complex General Relativity

Pseudo-complex general relativity and the slow rotation approximation for neutron stars

2019 ◽  
Vol 340 (1-3) ◽  
pp. 205-208 ◽  
Author(s):  
G. L. Volkmer ◽  
M. Razeira ◽  
D. Hadjimichef ◽  
F. Köpp ◽  
C. A. Z. Vasconcellos ◽  
...  
Keyword(s):  
General Relativity ◽  
Neutron Stars ◽  
Slow Rotation ◽  
Complex General Relativity

Pseudo-complex General Relativity and Neutron Stars

2014 ◽  
pp. 255-264
Author(s):  
Peter O. Hess ◽  
Isaac Rodríguez ◽  
Walter Greiner
Keyword(s):  
General Relativity ◽  
Neutron Stars ◽  
Complex General Relativity

scholarly journals Ray-tracing in pseudo-complex General Relativity

2014 ◽  
Vol 442 (1) ◽  
pp. 121-130 ◽  
Author(s):  
T. Schönenbach ◽  
G. Caspar ◽  
P. O. Hess ◽  
T. Boller ◽  
A. Müller ◽  
...  
Keyword(s):  
General Relativity ◽  
Ray Tracing ◽  
Complex General Relativity

scholarly journals Neutron stars as probes of dark matter

2020 ◽  
Vol 29 (14) ◽  
pp. 2043028
Author(s):  
M. Ángeles Pérez-García ◽  
Joseph Silk
Keyword(s):  
General Relativity ◽  
Dark Matter ◽  
Equation Of State ◽  
Neutron Stars ◽  
Internal Structure ◽  
Stellar Objects ◽  
Ordinary Matter ◽  
Stable Solutions ◽  
The Universe

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. However there is now a large consensus that an elusive sector of matter in the universe, described as dark matter, remains as yet undiscovered. In such a case, NSs should contain both, baryonic and dark matter. We argue that depending on the nature of the dark matter and in certain circumstances, the two matter components would form a mixture inside NSs that could trigger further changes, some of them observable. The very existence of NSs constrains the nature and interactions of dark matter in the universe.

The stellar graveyard

2019 ◽  
pp. 177-206
Author(s):  
Nils Andersson
Keyword(s):  
Black Holes ◽  
General Relativity ◽  
Neutron Stars ◽  
Gravitational Wave ◽  
Stellar Evolution ◽  
White Dwarfs ◽  
Supermassive Black Holes ◽  
Compact Objects ◽  
Fermi Gases ◽  
The 1950S

This chapter introduces the different classes of compact objects—white dwarfs, neutron stars, and black holes—that are relevant for gravitational-wave astronomy. The ideas are placed in the context of developing an understanding of the likely endpoint(s) of stellar evolution. Key ideas like Fermi gases and the Chandrasekhar mass are discussed, as is the emergence of general relativity as a cornerstone of astrophysics in the 1950s. Issues associated with different formation channels for, in particular, black holes are considered. The chapter ends with a discussion of the supermassive black holes that are found at the centre of galaxies.

Sign in / Sign up

Export Citation Format

Share Document