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As it is well-known that the hydrodinamic collapse of the massive star iron core should lead to the production of a hot neutron star. The assumption is made that the thermonuclear burning of the envelope matter, accreting onto the hot…

天体物理学 · 物理学 2009-10-31 S. S. Gershtein

It is shown that space curvature can be disposed of by properly taking into account gravitational self energies. This leads to a parameter free modification of Newton's law, violating Gauss theorem, which accounts for the crucial tests of…

综合物理 · 物理学 2011-12-09 Paolo Christillin

We exploit the fact that General Theory of Relativity (GTR) predicts the existence of compact objects having surface gravitational redshift z_s < =z_c=0.615 when the Equation of State (EOS) has the stringest general constraint that the…

天体物理学 · 物理学 2007-05-23 Abhas Mitra

The energy source has remained to be the great mystery in understanding of the gamma-ray bursts (GRBs) if the events are placed at cosmological distances as indicated by a number of recent observations. The currently popular models include…

天体物理学 · 物理学 2009-10-30 Bo Qin , Xiang-Ping Wu , Ming-Chung Chu , Li-Zhi Fang , Jing-Yao Hu

It is understood that the Supernovae (SNe) associated to Gamma Ray Bursts (GRBs) are of type Ib/c. The temporal coincidence of the GRB and the SN represents still a major enigma of Relativistic Astrophysics. We elaborate here, from the…

高能天体物理现象 · 物理学 2014-03-28 Jorge A. Rueda , Remo Ruffini

Gamma-Ray Bursts (GRBs) are extra-galactic and extremely energetic transient emissions of gamma rays, which are thought to be associated with the death of massive stars or the merger of compact objects in binary systems. Their huge…

高能天体物理现象 · 物理学 2016-07-20 F. Piron

We study the gravitational collapse of a spherically symmetric anisotropic relativistic star within Einstein theory of gravity making use of one of our recently developed collapsing stellar models [{\it Astrophys. Space Sci.} {\bf361} 99…

广义相对论与量子宇宙学 · 物理学 2022-01-05 Shyam Das , Bikash Chandra Paul , Ranjan Sharma

Gamma Ray Bursts (GRBs) are the most relativistic objects known so far, involving, on one hand an ultra-relativistic motion with a Lorentz factor $\Gamma > 100$ and on the other hand an accreting newborn black hole. The two main routes…

天体物理学 · 物理学 2007-05-23 Tsvi Piran

Dark Energy is the dominant component of the energy density of the universe. In a previous paper, we have shown that the collapse of dark energy fields leads to the formation of Super Massive Black Holes with masses comparable to the masses…

综合物理 · 物理学 2020-02-26 Vishal Jhalani , Ayushi Mishra , Anupam Singh

Cosmological GRBs are discussed with an emphasis on their plausible connection with black holes. GRBs can be triggered by collapse of stellar-mass objects that leads to formation of a black hole and a transient debris disk with a huge…

天体物理学 · 物理学 2008-11-26 Andrei M. Beloborodov

Repulsive interactions between neutrons in compact stellar cores cause luminosity and a steady outflow of hydrogen from stellar surfaces. Neutron repulsion in more massive compact objects made by gravitational collapse produces violent,…

核理论 · 物理学 2007-05-23 O. Manuel , Michael Mozina , Hilton Ratcliffe

The tidal disruption of a solar mass star around a supermassive black hole has been extensively studied analytically and numerically. In these events the star develops into an elongated banana-shaped structure. After completing an eccentric…

Observations show that at least some gamma-ray bursts (GRBs) happen simultaneously with core-collapse supernovae (SNe), thus linking by a common thread nature's two grandest explosions. We review here the growing evidence for and…

天体物理学 · 物理学 2008-11-26 S. E. Woosley , J. S. Bloom

It is now recognized that long-duration Gamma-Ray Bursts (GRBs) are linked to the collapse of massive stars, based on the association between (low-redshift) GRBs and (type Ic) core-collapse supernovae (SNe). The census of massive stars and…

Hypermassive neutron stars (HMNSs) -- equilibrium configurations supported against collapse by rapid differential rotation -- are possible transient remnants of binary neutron star mergers. Using newly developed codes for…

天体物理学 · 物理学 2008-11-26 Matthew D. Duez , Yuk Tung Liu , Stuart L. Shapiro , Masaru Shibata , Branson C. Stephens

A diverse range of phenomena is possible when a black hole experiences very rapid accretion from a disk due to the incomplete explosion of a massive presupernova star endowed with rotation. In the most extreme case, the outgoing shock fails…

天体物理学 · 物理学 2007-05-23 S. E. Woosley , A. I. MacFadyen , A. Heger

This short review is addressed to cosmologists. General relativity predicts that space-time comes to an end and physics comes to a halt at the big-bang. Recent developments in loop quantum cosmology have shown that these predictions cannot…

广义相对论与量子宇宙学 · 物理学 2011-01-25 Abhay Ashtekar

Using the Sparling form and a geometric construction adapted to spacetimes with a 2-dimensional isometry group, we analyse a quasi-local measure of gravitational energy. We then study the gravitational radiation through spacetime junctions…

广义相对论与量子宇宙学 · 物理学 2018-11-27 Alfonso García-Parrado , Filipe C. Mena

We study the collapse of a self-gravitating and radiating shell. Matter constituting the shell is quantized and the construction is viewed as a semiclassical model of possible black hole formation. It is shown that the shell internal…

广义相对论与量子宇宙学 · 物理学 2008-11-26 G. L. Alberghi , R. Casadio , G. P. Vacca , G. Venturi

A cloud of gas collapsing under gravity will fragment. We present a new theory for this process, in which layers shocked gas fragment due to their gravitational instability. Our model explains why angular momentum does not inhibit the…

天体物理学 · 物理学 2011-04-28 M. Wilkinson , B. Mehlig , M. A. Morgan