We report a series of exact cosmological solutions of the gravitational (1 + 1)-dimensional equations with a classical scalar field and an isotropic perfect fluid source. We consider a Robertson-Walker universe and obtain the scale factor and the field for several physically interesting potentials. In the case of a non-vanishing positive cosmological constant LAMBDA, we have found asymptotically de Sitter solutions which resemble the (3 + 1)-dimensional results, When LAMBDA = 0 we have to take restrictive conditions on the sip of the potential function in order to obtain exactly solvable models which include exponential inflationary processes.
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UNIV BUENOS AIRES, FAC CIENCIAS EXACTAS & NAT,DEPT FIS,PABELLON I, RA-1428 BUENOS AIRES, ARGENTINAUNIV BUENOS AIRES, FAC CIENCIAS EXACTAS & NAT,DEPT FIS,PABELLON I, RA-1428 BUENOS AIRES, ARGENTINA
CHIMENTO, LP
;
COSSARINI, AE
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UNIV BUENOS AIRES, FAC CIENCIAS EXACTAS & NAT,DEPT FIS,PABELLON I, RA-1428 BUENOS AIRES, ARGENTINAUNIV BUENOS AIRES, FAC CIENCIAS EXACTAS & NAT,DEPT FIS,PABELLON I, RA-1428 BUENOS AIRES, ARGENTINA
机构:
UNIV BUENOS AIRES, FAC CIENCIAS EXACTAS & NAT,DEPT FIS,PABELLON I, RA-1428 BUENOS AIRES, ARGENTINAUNIV BUENOS AIRES, FAC CIENCIAS EXACTAS & NAT,DEPT FIS,PABELLON I, RA-1428 BUENOS AIRES, ARGENTINA
CHIMENTO, LP
;
COSSARINI, AE
论文数: 0引用数: 0
h-index: 0
机构:
UNIV BUENOS AIRES, FAC CIENCIAS EXACTAS & NAT,DEPT FIS,PABELLON I, RA-1428 BUENOS AIRES, ARGENTINAUNIV BUENOS AIRES, FAC CIENCIAS EXACTAS & NAT,DEPT FIS,PABELLON I, RA-1428 BUENOS AIRES, ARGENTINA