We compute the spectrum of relic gravitons in a model of string cosmology. In the low- and in the high-frequency limits we reproduce known results. The full spectrum, however, also displays a series of oscillations which could give a characteristic signature at the planned LIGO/VIRGO detectors. For special values of the parameters of the model the signal reaches its maximum already at frequencies accessible to LIGO and VIRGO and it is close to the sensitivity of first generation experiments
The sensitivity achievable by a pair of VIRGO detectors to stochastic and isotropic gravitational wa...
The sensitivity achievable by a pair of VIRGO detectors to stochastic and isotropic gravitational wa...
A stochastic background of gravitational waves is expected to arise froma superposition of a large n...
We compute the spectrum of relic gravitons in a model of string cosmology. In the low- and in the hi...
We compute the spectrum of relic gravitons in a model of string cosmology. In the low- and in the hi...
A characteristic spectrum of relic gravitational radiation is produced by a period of “stringy infla...
A large class of string-cosmology backgrounds leads to a spectrum of relic stochastic gravitational ...
A large class of string-cosmology backgrounds leads to a spectrum of relic stochastic gravitational ...
A characteristic spectrum of relic gravitational radiation is produced by a period of “stringy infla...
Using general arguments we determine the allowed region for the end point frequency and the peak ene...
String cosmology models predict a stochastic cosmic background of gravitational waves with a charact...
n this paper, after discussing the mechanism of graviton production during an early phase of acceler...
This thesis shows the results of the search for gravitational-wave signals produced by cosmic string...
An exact analytic calculation is presented for the spectrum of relic gravitational waves in the scen...
We propose to uncover the signature of a stringy era in the primordial Universe by searching for a p...
The sensitivity achievable by a pair of VIRGO detectors to stochastic and isotropic gravitational wa...
The sensitivity achievable by a pair of VIRGO detectors to stochastic and isotropic gravitational wa...
A stochastic background of gravitational waves is expected to arise froma superposition of a large n...
We compute the spectrum of relic gravitons in a model of string cosmology. In the low- and in the hi...
We compute the spectrum of relic gravitons in a model of string cosmology. In the low- and in the hi...
A characteristic spectrum of relic gravitational radiation is produced by a period of “stringy infla...
A large class of string-cosmology backgrounds leads to a spectrum of relic stochastic gravitational ...
A large class of string-cosmology backgrounds leads to a spectrum of relic stochastic gravitational ...
A characteristic spectrum of relic gravitational radiation is produced by a period of “stringy infla...
Using general arguments we determine the allowed region for the end point frequency and the peak ene...
String cosmology models predict a stochastic cosmic background of gravitational waves with a charact...
n this paper, after discussing the mechanism of graviton production during an early phase of acceler...
This thesis shows the results of the search for gravitational-wave signals produced by cosmic string...
An exact analytic calculation is presented for the spectrum of relic gravitational waves in the scen...
We propose to uncover the signature of a stringy era in the primordial Universe by searching for a p...
The sensitivity achievable by a pair of VIRGO detectors to stochastic and isotropic gravitational wa...
The sensitivity achievable by a pair of VIRGO detectors to stochastic and isotropic gravitational wa...
A stochastic background of gravitational waves is expected to arise froma superposition of a large n...