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FIZIKA B 18 (2009) 4, 227-242
 
BIANCHI TYPE-I MAGNETIZED STIFF FLUID MODELS IN LYRA GEOMETRY
RAJ BALIa and NARESH K. CHANDNANIb
aDepartment of Mathematics, University of Rajasthan, Jaipur-302004,
India
E-mail address: balir5@yahoo.co.in
bDepartment of Mathematics, Jaipur Engineering College, Jaipur India
E-mail address:
chandnaninaresh1980@yahoo.co.in
Received 5 August 2009; Accepted 9 December 2009
Online 15 December 2009
Bianchi type-I magnetized cosmological models with time-dependent gauge
function b for stiff fluid distribution within the
framework of Lyra geometry are investigated. To get the deterministic model of
the universe, we have assumed that eigenvalue (s11)
of shear tensor (sij) is
proportional to the expansion (q). This leads to
A=(BC)n where A, B and C are metric potentials. The physical and
geometrical aspects of the models and singularities in the models are discussed.
PACS numbers: 04.50-h, 98.80-k
UDC 524.83, 52.423
Keywords: Bianchi type-I cosmological models, magnetized, stiff fluid, Lyra
geometry
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