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Supersymmetry of FRW barotropic cosmologies
HARET CODRATIAN ROSU
PEDRO ARMANDO OJEDA MAY
Acceso Abierto
Atribución-NoComercial-SinDerivadas
https://doi.org/10.1007/s10773-006-9123-2
Supersymmetry
FRW barotropic cosmology
Riccati equation
"Barotropic FRW cosmologies are presented from the standpoint of nonrelativis-tic supersymmetry. First, we reduce the barotropic FRW system of differential equations to simple harmonic oscillator differential equations. Employing the fac-torization procedure, the solutions of the latter equations are divided into the two classes of bosonic (nonsingular) and fermionic (singular) cosmological solutions. We next introduce a coupling parameter denoted by K between the two classes of solutions and obtain barotropic cosmologies with dissipative features acting on the scale factors and spatial curvature of the universe. The K-extended FRW equations in comoving time are presented in explicit form in the low coupling regime. The standard barotropic FRW cosmologies correspond to the dissipa-tionless limit K = 0."
Springer Link
2006
Artículo
Inglés
Público en general
Rosu, H.C. & Ojeda-May, P. Int J Theor Phys (2006) 45: 1152. https://doi.org/10.1007/s10773-006-9123-2
CIENCIAS FÍSICO MATEMÁTICAS Y CIENCIAS DE LA TIERRA
Versión aceptada
acceptedVersion - Versión aceptada
Aparece en las colecciones: Publicaciones Científicas Nanociencias y Materiales

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