Eric W. Weisstein.
General Relativity.
scienceworld.wolfram.com: Eric Weisstein's world of physics,
2005.
Web site, including many links to information about Einstein and
General Relativity.
LIGO Scientific Collaboration.
Detector description and performance for the first coincidence
observations between LIGO and GEO.
Nucl.Instrum.Meth., A517:154, 2004.
preprint.
Jolien Creighton.
Sound of LIGO (.au format 126KB).
This sound file was created from the AS_Q (antisymmetric port
quadrature) channel of one of the LIGO detectors, where a gravitational wave
signal would appear in the detector's output. To make this clip, the channel
has been bandpass filtered to restrict the sounds to the frequency range from
200 to 300 Hz.
Image from a simulation by Chad Hanna and Benjamin Owen.
Oscillating star.
from B. J. Owen's research page, Penn State University: An r-mode of
a rotating neutron star.
Fermi National Accelerator Laboratory (Fermilab).
What is the world made of?.
Fermilab inquiring minds: the science of matter, space and
time, 2004.
Explanation of quarks and elementary particles.
LIGO Scientific Collaboration.
Setting upper limits on the strength of periodic gravitational waves
using the first science data from the GEO 600 and LIGO detectors.
Physical Review D, 69:082004, 2004.
preprint.
LIGO Scientific Collaboration.
Upper limits on the strength of periodic gravitational waves from
PSR J1939+2134.
Classical and Quantum Gravity, 21:S671, 2004.
preprint.
Xavier Siemens, Bruce Allen, Jolien Creighton, Martin Hewitson, and
Michael Landry.
Making h(t) for LIGO.
Classical and Quantum Gravity, 21:S1723, 2004.
preprint.
P. Jaranowski, A. Królak, and B. F. Schutz.
Data analysis of gravitational-wave signals from spinning neutron
stars I. The signal and its detection.
Physical Review D, 58:063001, 1998.
preprint.