Gravo-thermal catastrophe in gravitational collapse and energy progenitor of Gamma-Ray Bursts

نویسندگان

چکیده

We study the homologous collapse of stellar nuclear core, virial theorem for hadron collisional relaxations, and photon productions from collisions. thus show gravo-thermal dynamical process that transforms gravitational energy to energy. The is energetically entropically favourable. total baryon number conservation, Euler equation energy-momentum conservation Poisson's potential are adopted describe core collapses. determines collision gain potential. hadronic production rate density. time scales macroscopic microscopic processes studied verify approximations. As a result, we formation opaque photon-pair spheres, whose energy, size, temperature density, accounting main energetic features Gamma-Ray Burst progenitors. obtain intrinsic correlations these quantities. They depend only on averaged thermal index core. discuss possibility confront them with observational data.

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Gravitational collapse as the source of gamma - ray bursts 1

If the threshold for e − e + pair production depends on an angle between photon momenta, and if the γ-rays are collimated right in gamma-ray burst (GRB) source then another solution of the compactness problem is possible. The list of basic assumptions of the scenario describing the GRB with energy release < 10 49 erg is adduced: the matter is about an alternative to the ultrarelativis-tic fireb...

متن کامل

The Progenitor Stars of Gamma-Ray Bursts

Those massive stars that, during their deaths, give rise to gamma-ray bursts (GRBs) must be endowed with an unusually large amount of angular momentum in their inner regions, one to two orders of magnitude greater than the ones that make common pulsars. Yet the inclusion of mass loss and angular momentum transport by magnetic torques during the precollapse evolution is known to sap the core of ...

متن کامل

Gravitational Waves from Gamma-ray Bursts

We present a mechanism for long bursts of gravitational radiation from Kerr black holes surrounded by a torus. These systems are believed to form in core-collapse of massive stars in association with gamma-ray bursts. The torus cat-alyzes black hole-spin energy mostly into gravitational radiation, with a minor output in winds, thermal and neutrino emissions. Torus winds impact the remnant envel...

متن کامل

Polarized Gravitational Waves from Gamma-Ray Bursts

Significant gravitational wave emission is expected from gamma-ray bursts arising from compact stellar mergers, and possibly also from bursts associated with fast-rotating massive stellar core collapses. These models have in common a high angular rotation rate, and observations provide evidence for jet collimation of the photon emission, with properties depending on the polar angle. Here we con...

متن کامل

Gravitational Radiation from Gamma-Ray Bursts∗

Gamma Ray Bursts (GRBs) are the most relativistic objects known so far, involving, on one hand an ultra-relativistic motion with a Lorentz factor Γ > 100 and on the other hand an accreting newborn black hole. The two main routes leading to this scenario: binary neutron star mergers and Collapsar the collapse of a rotating star to a black hole, are classical sources for gravitational radiation. ...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: Journal of Cosmology and Astroparticle Physics

سال: 2021

ISSN: ['1475-7516', '1475-7508']

DOI: https://doi.org/10.1088/1475-7516/2021/07/044