Pregled bibliografske jedinice broj: 941202
Tachyon with an inverse power-law potential in a braneworld cosmology
Tachyon with an inverse power-law potential in a braneworld cosmology // Classical and Quantum Gravity, 34 (2017), 16; 165006, 19 doi:10.1088/1361-6382/aa7e0f (međunarodna recenzija, članak, znanstveni)
CROSBI ID: 941202 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
Tachyon with an inverse power-law potential in a braneworld cosmology
Autori
Bilić, Nevenko ; Domazet, Silvije ; Djordjevic, Goran S.
Izvornik
Classical and Quantum Gravity (0264-9381) 34
(2017), 16;
165006, 19
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
tachyon ; braneworld cosmology ; Randall–Sundrum model
Sažetak
We study a tachyon cosmological model based on the dynamics of a 3-brane in the bulk of the second Randall–Sundrum model extended to more general warp functions. A well known prototype of such a generalization is the bulk with a selfinteracting scalar field. As a consequence of a generalized bulk geometry the cosmology on the observer brane is modified by the scale dependent four-dimensional gravitational constant. In particular, we study a power law warp factor which generates an inverse power-law potential $V\propto \varphi^{; ; -n}; ; $ of the tachyon field phiv. We find a critical power n cr that divides two subclasses with distinct asymptotic behaviors: a dust universe for $n>n_{; ; \rm cr}; ; $ and a quasi de Sitter universe for $0<n<n_{; ; \rm cr}; ; $ .
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA
Ustanove:
Institut "Ruđer Bošković", Zagreb
Citiraj ovu publikaciju:
Časopis indeksira:
- Current Contents Connect (CCC)
- Web of Science Core Collection (WoSCC)
- Science Citation Index Expanded (SCI-EXP)
- SCI-EXP, SSCI i/ili A&HCI
- Scopus