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Associate Professor Jolien Creighton
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jolien@gravity.phys.uwm.edu
Personal Home Page
Telephone: (414) 229-2907
Room: 474
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Jolien Creighton's interests are in the General
Relativistic theory of gravity, with a focus on the physics of
black holes and gravitational wave radiation. His scientific
goal is to use gravitational radiation to observe colliding
black holes (and other sources of gravitational radiation) in
the distant universe.
Gravitational waves -- oscillating gravitational fields that cause the distance
between neighboring points to stretch and shrink -- are expected to be
propagating throughout space, but, since the force of gravity is relatively
weak, these waves barely interact with matter and travel through the earth (and
us) unnoticed. The strongest gravitational waves will likely come from
cataclysmic events, such as the collisions of massive black holes, but even
these strongest sources will only produce a miniscule effect here on the earth.
A major US project to observe gravitational waves called the Laser
Interferometric Gravitational-wave Observatory (LIGO) has been constructed and
is now beginning to operate. The two LIGO observatories in Hanford, Washington
and Livingston, Louisiana, use laser interferometry to monitor the relative
distances between mirrors in two orthogonal optical cavities that are four
kilometers long. LIGO was designed to be able to detect a gravitational wave
that produces a change of a thousandth of the size of an atomic nucleus in the
distance between the mirrors at the ends of the cavities.
Creighton's goals are to use the data obtained from LIGO and other
gravitational wave observatories to detect the astrophysical events that
produce gravitational waves, and to use the observations to learn about the
sources of the waves and the nature of strong gravity. This work involves
modeling various strong sources of gravitational waves, such as black hole
collisions, to obtain the expected signal, which is needed so that the
astrophysical events can be discerned from the instrument noise. Observations
of black hole collisions will yield important information about the black hole
population in the universe and about the strong gravitational field in the
vicinity of a black hole.
Jolien Creighton was an undergraduate at the University of Calgary, graduating
in 1992 with a B.Sc. in Physics with a minor in Astrophysics. At the
University of Calgary, Creighton studied supernova remnants and X-ray binary
systems using radio and X-ray observations. He did his graduate work on the
thermodynamics of black holes at the University of Waterloo, and received his
Ph.D. in 1996. Creighton then worked as a postdoctoral scholar at the
California Institute of Technology and the University of Wisconsin --
Milwaukee, where he became involved in the LIGO project and developed methods
for detecting black holes using gravitational wave observations. He was
appointed to the UWM faculty in 2002.
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