E-viri
Recenzirano
Odprti dostop
-
Buonanno, Alessandra; Sigl, Günter; Raffelt, Georg G.; Janka, Hans-Thomas; Müller, Ewald
Physical review. D, Particles, fields, gravitation, and cosmology, 10/2005, Letnik: 72, Številka: 8Journal Article
Based on new developments in the understanding of supernovae as gravitational-wave (GW) sources, we estimate the GW background from all cosmic supernovae. While our estimate is uncertain within a few orders of magnitude, this background may become detectable by second-generation space-based interferometers such as the proposed Big-Bang Observatory. At frequencies below about 1 Hz this GW background is stochastic. Down to about 0.01 Hz it could well be of comparable magnitude to the one expected from standard inflationary models, especially in the presence of an early population of massive stars.
![loading ... loading ...](themes/default/img/ajax-loading.gif)
Vnos na polico
Trajna povezava
- URL:
Faktor vpliva
Dostop do baze podatkov JCR je dovoljen samo uporabnikom iz Slovenije. Vaš trenutni IP-naslov ni na seznamu dovoljenih za dostop, zato je potrebna avtentikacija z ustreznim računom AAI.
Leto | Faktor vpliva | Izdaja | Kategorija | Razvrstitev | ||||
---|---|---|---|---|---|---|---|---|
JCR | SNIP | JCR | SNIP | JCR | SNIP | JCR | SNIP |
Baze podatkov, v katerih je revija indeksirana
Ime baze podatkov | Področje | Leto |
---|
Povezave do osebnih bibliografij avtorjev | Povezave do podatkov o raziskovalcih v sistemu SICRIS |
---|
Vir: Osebne bibliografije
in: SICRIS
To gradivo vam je dostopno v celotnem besedilu. Če kljub temu želite naročiti gradivo, kliknite gumb Nadaljuj.