The Lense-Thirring effect first pointed out by Lense (1917) and Thirring (1918) in
connection with the precession of the orbital plane of an orbiting body around a rotating
mass within Einstein's theory of gravity, then in its infancy, remains even today the
source of a variety of fundamental theoretical and experimental/observational questions.
This spin-orbital angular momentum coupling of the gravitational interaction is one of a
number of related issues involving the behavior of test bodies around rotating masses
which will be explored in this first ICRA workshop confronting theory with both experiment
and observation in the spirit of the previous two meetings honoring Bill Fairbank.
This general topic which has come to be known as gravitomagnetism has seen considerable
progress in its understanding over the years, but there is still much to learn. Falling
under the wider umbrella of gravitoelectromagnetism, the analogy between the linear theory
of electromagnetism and linearized general relativity which extends to the nonlinear
regime through the introduction of test observer formalism, it has provided the stimulus
to develop a clearer picture of the theoretical framework of extending space-plus-time
language and concepts to strong field gravity. Among the novel ideas this has flushed out
has been some of the interesting properties of noninertial forces like the centrifugal
force within general relativity and related behavior of spinning test bodies. Although the
orbits of nonspinning particles in the stationary geometries of neutron stars and black
holes are rather well understood, we are still far from a complete understanding of the
behavior of spinning particles in gravitational fields and of the implications of the
different theoretical approaches to this problem. It is possible that analogies between
the treatment in quantum and classical electrodynamics might lead to clarification of
these issues.
After more than twenty years the Gravity Probe B project is finally nearing completion.
Meanwhile evidence has been reported of possible observations and measurements of the
Lense-Thirring effect by a satellite orbiting the Earth and in the strong gravitational
fields of neutron stars and black holes. The current status of these experiments and
observations will be reviewed critically and the merits if different approaches compared.
All those who have made major contributions to this field and are still with us will
be invited to participate in the meeting. Its proceedings including both the participant
talks and selected reprints from the past literature on the topic will be published in a
book of the World Scientific series "Advances in Astrophysics and Cosmology" edited
by Fang Li-Zhi and Remo Ruffini.
Topics will include the following:
- Equations of Motion of Spinning Particles in Electrodynamics and General Relativity
- Inertial Forces and Gravitoelectromagnetism
- The Stanford GP-B Mission: Status
- Probing the Gravitomagnetic Lens-Thirring Effect with the LAGEOS Satellite
- Probing the Gravitomagnetic Lens-Thirring Effect with Neutron Stars and Black Holes
- Assessment of Error Analysis
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