scholarly journals General Relativistic, Neutrino‐assisted Magnetohydrodynamic Winds—Theory and Application to Gamma‐Ray Bursts. I. Schwarzschild Geometry

2006 ◽  
Vol 648 (1) ◽  
pp. 510-522 ◽  
Author(s):  
Amir Levinson
Keyword(s):  
Gamma Ray ◽  
Gamma Ray Bursts ◽  
Schwarzschild Geometry ◽  
General Relativistic

General Relativistic Binary Merger Simulations and Short Gamma-Ray Bursts

2006 ◽  
Vol 641 (2) ◽  
pp. L93-L96 ◽  
Author(s):  
Joshua A. Faber ◽  
Thomas W. Baumgarte ◽  
Stuart L. Shapiro ◽  
Keisuke Taniguchi
Keyword(s):  
Gamma Ray ◽  
Gamma Ray Bursts ◽  
General Relativistic

scholarly journals Advection schemes for capturing relativistic shocks with high Lorentz factors

10.4081/710 ◽  
2012 ◽  
Vol 2 (1) ◽  
pp. e1
Author(s):  
Ahmad A. Hujeirat ◽  
Sophie Fehlmann
Keyword(s):  
Total Energy ◽  
Gamma Ray ◽  
Gamma Ray Bursts ◽  
Relativistic Plasmas ◽  
Advection Scheme ◽  
Numerical Studies ◽  
Relativistic Shocks ◽  
Advection Schemes ◽  
General Relativistic ◽  
Energy Formulation

Jet-plasmas emanating from the vicinity of relativistic objects and in gamma-ray bursts have been observed to propagate with Lorentz factors laying in the range between one and several hundreds. On the other hand, the numerical studies of such flows have been focused so far mainly on the lowest possible range of Lorentz factors Γ, specifically, on the regime 1 ≤ Γ ≤ 5. Therefore, relativistic flows with high Γ− factors have poorly studied, as most numerical methods are found to encounter severe numerical difficulties or even become numerically unstable for Γ >> 1. In this paper we present an implicit numerical advection scheme for modeling the propagation of relativistic plasmas with shocks, discuss its consistency with respect to both the internal and total energy formulation in general relativity. Using the total energy formulation, the scheme is found to be viable for modeling moving shocks with moderate Lorentz factors, though with relatively small Courant numbers. In the limit of high Lorentz factors, the internal energy formulation in combination with a fine-tuned artificial viscosity is much more robust and efficient. We confirm our conclusions by performing test calculations and compare the results with analytical solutions of the relativistic shock tube problem. The aim of the present modification is to enhance the robustness of the general relativistic implicit radiative MHD solver: GR-I-RMHD (http://www1.iwr.uni-heidelberg.de/groups/compastro/home/gr-i-mhdsolver) and extend its range of applications into the high Γ− regime.

scholarly journals Advection schemes for capturing relativistic shocks with high Lorentz factors

2012 ◽  
Vol 2 (1) ◽  
pp. e1
Author(s):  
Ahmad A. Hujeirat ◽  
Sophie Fehlmann
Keyword(s):  
Total Energy ◽  
Gamma Ray ◽  
Gamma Ray Bursts ◽  
Relativistic Plasmas ◽  
Advection Scheme ◽  
Numerical Studies ◽  
Relativistic Shocks ◽  
Advection Schemes ◽  
General Relativistic ◽  
Energy Formulation

Jet-plasmas emanating from the vicinity of relativistic objects and in gamma-ray bursts have been observed to propagate with Lorentz factors laying in the range between one and several hundreds. On the other hand, the numerical studies of such flows have been focused so far mainly on the lowest possible range of Lorentz factors Γ, specifically, on the regime 1 ≤ Γ ≤ 5. Therefore, relativistic flows with high Γ− factors have poorly studied, as most numerical methods are found to encounter severe numerical difficulties or even become numerically unstable for Γ >> 1. In this paper we present an implicit numerical advection scheme for modeling the propagation of relativistic plasmas with shocks, discuss its consistency with respect to both the internal and total energy formulation in general relativity. Using the total energy formulation, the scheme is found to be viable for modeling moving shocks with moderate Lorentz factors, though with relatively small Courant numbers. In the limit of high Lorentz factors, the internal energy formulation in combination with a fine-tuned artificial viscosity is much more robust and efficient. We confirm our conclusions by performing test calculations and compare the results with analytical solutions of the relativistic shock tube problem. The aim of the present modification is to enhance the robustness of the general relativistic implicit radiative MHD solver: GR-I-RMHD (http://www1.iwr.uni-heidelberg.de/groups/compastro/home/gr-i-mhdsolver) and extend its range of applications into the high Γ− regime.

scholarly journals GAMMA-RAY BURSTS AS THE BIRTH-CRIES OF BLACK HOLES

2000 ◽  
Vol 15 (15) ◽  
pp. 991-995 ◽  
Author(s):  
PANKAJ S. JOSHI ◽  
NARESH K. DADHICH ◽  
ROY MAARTENS
Keyword(s):  
Black Holes ◽  
Black Hole ◽  
Gamma Ray ◽  
Massive Stars ◽  
Relativistic Effects ◽  
Gamma Ray Bursts ◽  
Trapped Surfaces ◽  
General Relativistic

The origin of cosmic gamma-ray bursts remains one of the most intriguing puzzles in astronomy. We suggest that purely general relativistic effects in the collapse of massive stars could account for these bursts. The late formation of closed trapped surfaces can occur naturally, allowing the escape of huge energy from curvature-generated fireballs, before these are hidden within a black hole.

Sign in / Sign up

Export Citation Format

Share Document