Gamma-ray Bursts,
and in particular the effects that the X-ray/UV radiation accompanying
them produce on their surrounding gas. This has led to the
development of a radiative transfer code that can
self-consistently track gas photoionization and dust destruction
by the burst radiation.
Other interests concern the physics of accretion disks accreting at
very high rates and cooling through neutrino emission. These are
believed to provide the ultimate source of power for GRBs.
Since the launch of the Swift satellite, I have also been working
towards understanding the origin of puzzling and unexpected phenomena,
such as the presence of X-ray flares in the early afterglow lightcurves.
Within the context of short GRBs, my research has focused on making
a connection between the theoretical predictions for the mergers
of two compact objects (neutron star-neutron star and neutron star-black hole),
and the observable properties of the resulting GRBs.
Neutron Stars,
with particular emphasis on Anomalous X-ray Pulsars and Soft Gamma-Ray
Repeaters, a subclass of neutron stars thought to be endowed with very
large magnetic fields (and also dubbed "magnetars"). Other interests
involve isolated, old neutron stars accreting from the interstellar
medium, the connection between pulsars and HI supershells, the spin
periods of neutron stars at birth, and
the timing behaviour of accreting X-ray Binaries.
Cosmology
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research topics include:
Gravitational Lensing
and Microlensing, the
latter
with focus on
microlensing by stars in binaries.
Interstellar Medium
(ISM), and in particular the use of Gamma-Ray Bursts
as probes of the ISM in high-redshift galaxies.
Foregrounds for
measurements of the Cosmic Microwave Background
and for 21-cm experiments. Particular focus has been on the
contaminating
signal from the radio-emitting centers of nearby, early-type galaxies.