1,442 research outputs found
A Theory of Mulicolor Black Body Emission from Relativistically Expanding Plasmas
We consider the emission of photons from the inner parts of a
relativistically expanding plasma outflow, characterized by a constant Lorentz
factor, Gamma. Photons that are injected in regions of high optical depth are
advected with the flow until they escape at the photosphere. Due to multiple
scattering below the photosphere, the locally emerging comoving photon
distribution is thermal. However, as an observer sees simultaneously photons
emitted from different angles, hence with different Doppler boosting, the
observed spectrum is a multi-color black-body. We calculate here the properties
of the observed spectrum at different observed times. Due to the strong
dependence of the photospheric radius on the angle to the line of sight, for
parameters characterizing gamma-ray bursts (GRBs) thermal photons are seen up
to tens of seconds following the termination of the inner engine. At late
times, following the inner engine termination, both the number flux and energy
flux of the thermal spectrum decay as F ~ t^{-2}. At these times, the
multicolor black body emission results in a power law at low energies (below
the thermal peak), with power law index F_\nu ~ \nu^{0}. This result is
remarkably similar to the average value of the low energy spectral slope index
(``\alpha'') seen in fitting the spectra of large GRB sample.Comment: 8 pages, 2 figures; submitted for publication in Ap.
Dynamical Model of an Expanding Shell
Expanding blast waves are ubiquitous in many astronomical sources, such as
supernovae remnants (SNRs), X-ray emitting binaries (XRBs) and gamma-ray bursts
(GRBs). I consider here the dynamics of such an expanding blast wave, both in
the adiabatic and the radiative regimes. As the blast wave collects material
from the surrounding, it decelerates. A full description of the temporal
evolution of the blast wave requires consideration of both the energy density
and the pressure of the shocked material. The obtained equation is different
than earlier works in which only the energy was considered. The solution
converges to the familiar results in both the ultra-relativistic and the
sub-relativistic (Newtonian) regimes.Comment: Minor revision. Some points clarified, references added. Accepted for
publication in Ap.J. (Lett.
Constraining Magnetization of Gamma-Ray Bursts Outflows using Prompt Emission Fluence
I consider here acceleration and heating of relativistic outflow by local
magnetic energy dissipation process in Poynting flux dominated outflow.
Adopting the standard assumption that the reconnection rate scales with the
Alfven speed, I show here that the fraction of energy dissipated as thermal
photons cannot exceed (13 % (for adiabatic index
) of the kinetic energy at the photosphere. Even in the most
radiatively efficient scenario, the energy released as non-thermal photons
during the prompt phase is at most equal to the kinetic energy of the outflow.
These results imply that calorimetry of the kinetic energy that can be done
during the afterglow phase, could be used to constrain the magnetization of
gamma-ray bursts (GRB) outflows. I discuss the recent observational status, and
its implications on constraining the magnetization in GRB outflows.Comment: (Very) extensive discussions about current observational constraints,
implications and limitations. Accepted for publication in the Astrophysical
Journa
Radiative Mechanisms in GRB prompt emission
Motivated by the Fermi gamma-ray space telescope results, in recent years
immense efforts were given to understanding the mechanism that leads to the
prompt emission observed. The failure of the optically thin emission models
(synchrotron and synchrotron self Compton) increased interest in alternative
models. Optically thick models, while having several advantages, also face
difficulty in capturing several key observables. Theoretical efforts are
focused in two main directions: (1) mechanisms that act to broaden the Planck
spectrum; and (2) combining the optically thin and optically thick models to a
hybrid model that could explain the key observables.Comment: 9 pages, 2 figures, 1 table; Invited review, to appear in the
proceedings of the Gamma-Ray Burst Symposium 2012- IAA-CSIC - Marbella,
editors: Castro-Tirado, A. J., Gorosabel, J. and Park, I.
Plasmas in Gamma-Ray Bursts: particle acceleration, magnetic fields, radiative Processes and environments
Being the most extreme explosions in the universe, gamma-ray bursts (GRBs)
provide a unique laboratory to study various plasma physics phenomena. The
complex lightcurve and broad-band, non-thermal spectra indicate a very
complicated system on the one hand, but on the other hand provide a wealth of
information to study it. In this chapter I focus on recent progress in some of
the key unsolved physical problems. These include: (1) Particle acceleration
and magnetic field generation in shock waves; (2) Possible role of strong
magnetic fields in accelerating the plasmas, and accelerating particles via
magnetic reconnection process; (3) Various radiative processes that shape the
observed lightcurve and spectra, both during the prompt and the afterglow
phases, and finally (4) GRB environments and their possible observational
signature.Comment: Invited chapter for a special issue of "galaxies", dedicated to
"Cosmic Plasmas and Electromagnetic phenomena
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