activity
19952007
most citedSensitivity curves for spaceborne gravitational wave interferometers

202 citations · 1k across the 27 of their papers we have counts for

collaborators

27 papers

gr-qc2007★ 2 cited

Effects of quantized fields on the spacetime geometries of static spherically symmetric black holes

Paul R. Anderson, Mathew Binkley, Hector Calderon +3

Analytic approximations for the stress-energy of quantized fields in the Hartle-Hawking state in static black hole spacetimes predict divergences on the event horizon of the black…

gr-qc2005★ 4 cited

Effects of nonzero neutrino masses on black hole evaporation

Daniel Bambeck, William A. Hiscock

We study the consequences of nonzero neutrino masses for black holes evaporating by the emission of Hawking radiation. We find that the evolution of small, hot, black holes may be…

gr-qc2004★ 25 cited

Quantum fields and "Big Rip" expansion singularities

Hector Calderon, William A. Hiscock

The effects of quantized conformally invariant massless fields on the evolution of cosmological models containing a ``Big Rip'' future expansion singularity are examined. Quantized…

physics.space-ph2002★ 2 cited

From Wormholes to the Warp Drive: Using theoretical physics to place ultimate bounds on technology

William A. Hiscock

The serious study of such science fiction staples as wormholes, time travel, and the warp drive, as a means of understanding and constraining possible realistic solutions within Ge…

gr-qc2002★ 47 cited

LISA, binary stars, and the mass of the graviton

Curt Cutler, William A. Hiscock, Shane L. Larson

We extend and improve earlier estimates of the ability of the proposed LISA (Laser Interferometer Space Antenna) gravitational wave detector to place upper bounds on the graviton m…

gr-qc2002★ 45 cited

Unequal arm space-borne gravitational wave detectors

Shane L. Larson, Ronald W. Hellings, William A. Hiscock

Unlike ground-based interferometric gravitational wave detectors, large space-based systems will not be rigid structures. When the end-stations of the laser interferometer are free…