I'm interested in the approximate analytical description of binary compact
objects in general relativity and its application future gravitational wave astronomy.
More specifically I am interested in the inclusion of higher multipoles of the
compact objects, such as spin or quadrupole, into the post-Newtonian or
post-Minkowskian approximations.
Abstract:
The inspiral of compact objects like black holes or neutron stars can
be approximated using point masses very well. However, very interesting
astronomical information is contained in effects to gravitational waves
arising from the object's higher multipoles (or their finite size).
Some of these effects can be modeled by an extension of the point mass
action. Based on such an action, contributions of dipole (i.e., spin)
and quadrupole to the post-Newtonian (PN) approximation can be
obtained. The quadrupole effects are the first which encode information
of the internal structure of the compact objects, e.g., they allow an
distinction between black holes and neutron stars and also different
equations of state.
Canonical formulation of spinning objects in general relativity from an action approach (Juli 5th, 2010)
Abstract:
An extension of the canonical formalism of Arnowitt, Deser, and Misner
from point-masses to spinning objects is presented.
The derivation of this extension is based on an action functional
and is similar to the original derivation of Arnowitt,
Deser, and Misner for non-spinning objects.
This action approach currently covers the pole-dipole approximation
of self-gravitating extended bodies to linear order in spin.
As an application, spin contributions to the conservative next-to-leading
order in the post-Newtonian approximation scheme are presented.
Also higher orders and radiation reaction effects in the Hamiltonian due to spin
are discussed.
Canonical formulation of spinning objects in general relativity (March 19th, 2010)
Abstract:
The extension of the canonical formalism of Arnowitt, Deser and
Misner from point-masses to spinning objects is a long standing problem in
General Relativity. Two independent approaches to a solution of this problem
are given in this talk. The first is based on an explicit order-by-order
construction of the canonical formalism within the post-Newtonian
approximation scheme. Here the global Poincare algebra is the important
consistency condition. The second approach is based on an action functional
and is similar to the original derivation of Arnowitt, Deser and Misner for
non-spinning objects. A comparison to the canonical formulation of the Dirac
field coupled to gravity is made. As an application, spin and quadrupole
contributions to next-to-leading order in the post-Newtonian approximation
scheme are presented.