Add to ORKGHigh-frequency gravitational waves can be detected by observing the frequency modulation they impart on photons. We discuss fundamental limitations to this method related to the fact that it is impossible to construct a perfectly rigid detector. We then propose several novel methods to search for O(MHz-GHz) gravitational waves based on the frequency modulation induced in the spectrum of an intense laser beam, by applying optical frequency demodulation techniques, or by using optical atomic clock technology. We find promising sensitivities across a broad frequency range.Comment: 11 pages, 3 figures. Matches journal versio
Within this decade gravitational wave detection will open a new observational window on the Universe...
It is suggested that gravity waves could, in several cases, be detected by means of already (or shor...
The direct detection of gravitational waves promises to open a new observational window onto the uni...
We study the graviton-photon conversion in the magnetic fields of the Earth, our galaxy, and interga...
In this work, we present the first experimental upper limits on the presence of stochastic gravitati...
Gravitational wave detection can be done by precision timing of millisecond pulsars, and (with less ...
We propose a space-based gravitational wave (GW) detector consisting of two spatially separated, dra...
High-frequency gravitational waves (HFGWs) carry a wealth of information on the early Universe with ...
Detecting gravitational waves with frequencies higher than 10 kHz requires new strategies. In previo...
Einstein's general theory of relativity predicts that accelerating mass distributions produce gravit...
The first direct measurement of gravitational waves by the LIGO and Virgo collaborations has opened ...
We describe the design of a gravitational wave timing array, a novel scheme that can be used to sear...
In this article, which will appear as a chapter in the Handbook of Gravitational Wave Astronomy, we ...
Stochastic gravitational wave background from the early Universe has a cut-off frequency close to 10...
In the presence of magnetic fields, gravitational waves are converted into photons and vice versa. W...
Within this decade gravitational wave detection will open a new observational window on the Universe...
It is suggested that gravity waves could, in several cases, be detected by means of already (or shor...
The direct detection of gravitational waves promises to open a new observational window onto the uni...
We study the graviton-photon conversion in the magnetic fields of the Earth, our galaxy, and interga...
In this work, we present the first experimental upper limits on the presence of stochastic gravitati...
Gravitational wave detection can be done by precision timing of millisecond pulsars, and (with less ...
We propose a space-based gravitational wave (GW) detector consisting of two spatially separated, dra...
High-frequency gravitational waves (HFGWs) carry a wealth of information on the early Universe with ...
Detecting gravitational waves with frequencies higher than 10 kHz requires new strategies. In previo...
Einstein's general theory of relativity predicts that accelerating mass distributions produce gravit...
The first direct measurement of gravitational waves by the LIGO and Virgo collaborations has opened ...
We describe the design of a gravitational wave timing array, a novel scheme that can be used to sear...
In this article, which will appear as a chapter in the Handbook of Gravitational Wave Astronomy, we ...
Stochastic gravitational wave background from the early Universe has a cut-off frequency close to 10...
In the presence of magnetic fields, gravitational waves are converted into photons and vice versa. W...
Within this decade gravitational wave detection will open a new observational window on the Universe...
It is suggested that gravity waves could, in several cases, be detected by means of already (or shor...
The direct detection of gravitational waves promises to open a new observational window onto the uni...