The gross features of gravitational radiation bathing the Earth from a set of a 330 + 4 PSR have been computed. Particular attention has been paid in evaluating the lower and upper bounds of gravitational wave background, in view of planning GW detection experiments in the frequency range 0.1 Hz - 1 kHz. The analysis seems to indicate that strain sensitivities of the order of 10-26 would allow the detection of several sparse PSR sources.

Gravitational wave background from a sample of 330 + 4 pulsars

BARONE, Fabrizio;
1988-01-01

Abstract

The gross features of gravitational radiation bathing the Earth from a set of a 330 + 4 PSR have been computed. Particular attention has been paid in evaluating the lower and upper bounds of gravitational wave background, in view of planning GW detection experiments in the frequency range 0.1 Hz - 1 kHz. The analysis seems to indicate that strain sensitivities of the order of 10-26 would allow the detection of several sparse PSR sources.
File in questo prodotto:
Non ci sono file associati a questo prodotto.

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11386/3782077
 Attenzione

Attenzione! I dati visualizzati non sono stati sottoposti a validazione da parte dell'ateneo

Citazioni
  • ???jsp.display-item.citation.pmc??? ND
  • Scopus ND
  • ???jsp.display-item.citation.isi??? 9
social impact