Add to ORKGCusps of cosmic strings emit strong beams of high-frequency gravitational waves (GW). As a consequence of these beams, the stochastic ensemble of gravitational waves generated by a cosmological network of oscillating loops is strongly non Gaussian, and includes occasional sharp bursts that stand above the rms GW background. These bursts might be detectable by the planned GW detectors LIGO/VIRGO and LISA for string tensions as small as $G \mu \sim 10^{-13}$. The GW bursts discussed here might be accompanied by Gamma Ray Bursts
Cosmic strings are topological defects which can be formed in grand unified theory scale phase trans...
Cosmic strings are topological defects which can be formed in grand unified theory scale phase trans...
International audienceIn the era of the next generation of gravitational wave experiments a stochast...
The strong beams of high-frequency gravitational waves (GW) emitted by cusps and kinks of cosmic str...
We consider the stochastic background of gravitational waves produced by a network of cosmic strings...
The mean spectrum and burst statistics of gravitational waves produced by a cosmological population ...
The gravitational wave (GW) signals emitted by a network of cosmic strings are reexamined in view of...
String cosmology models predict a stochastic cosmic background of gravitational waves with a charact...
The next generation of gravitational wave detectors holds out the prospect of detecting a stochastic...
Spectra of the stochastic gravitational wave backgrounds from cosmic strings are calculated and comp...
A large class of string-cosmology backgrounds leads to a spectrum of relic stochastic gravitational ...
We investigate the ability of the Laser Interferometer Space Antenna (LISA) to detect a stochastic g...
If cosmic strings are formed in the early universe, their associated loops emit gravitational waves ...
If cosmic strings are formed in the early universe, their associated loops emit gravitational waves ...
Cosmic strings are topological defects which can be formed in grand unified theory scale phase trans...
Cosmic strings are topological defects which can be formed in grand unified theory scale phase trans...
Cosmic strings are topological defects which can be formed in grand unified theory scale phase trans...
International audienceIn the era of the next generation of gravitational wave experiments a stochast...
The strong beams of high-frequency gravitational waves (GW) emitted by cusps and kinks of cosmic str...
We consider the stochastic background of gravitational waves produced by a network of cosmic strings...
The mean spectrum and burst statistics of gravitational waves produced by a cosmological population ...
The gravitational wave (GW) signals emitted by a network of cosmic strings are reexamined in view of...
String cosmology models predict a stochastic cosmic background of gravitational waves with a charact...
The next generation of gravitational wave detectors holds out the prospect of detecting a stochastic...
Spectra of the stochastic gravitational wave backgrounds from cosmic strings are calculated and comp...
A large class of string-cosmology backgrounds leads to a spectrum of relic stochastic gravitational ...
We investigate the ability of the Laser Interferometer Space Antenna (LISA) to detect a stochastic g...
If cosmic strings are formed in the early universe, their associated loops emit gravitational waves ...
If cosmic strings are formed in the early universe, their associated loops emit gravitational waves ...
Cosmic strings are topological defects which can be formed in grand unified theory scale phase trans...
Cosmic strings are topological defects which can be formed in grand unified theory scale phase trans...
Cosmic strings are topological defects which can be formed in grand unified theory scale phase trans...
International audienceIn the era of the next generation of gravitational wave experiments a stochast...