Growth rate of cosmological perturbations in standard model: Explicit analytical solution

Astronomy and Astrophysics

Volumn 399, Issue 1, 2003, Pages 19-21

  Chernin, A D ^a,b,c   Nagirner, D I ^d,e   Starikova, S V ^d  

^a MOSCOW STATE UNIVERSITY   (Russian Federation)

^b UNIVERSITY OF TURKU   (Finland)

^c UNIVERSITY OF OULU   (Finland)

^d ST PETERSBURG STATE UNIVERSITY   (Russian Federation)

^e ISAAC NEWTON INSTITUTE OF CHILE   (Chile)

Author keywords

Cosmology: large scale structure of Universe; Cosmology: theory

Indexed keywords

APPROXIMATION THEORY; FUNCTIONS; INTEGRAL EQUATIONS; PERTURBATION TECHNIQUES; POLYNOMIALS;

COSMOLOGICAL PERTURBATIONS; COSMOLOGY; LARGE-SCALE STRUCTURE OF UNIVERSE; NON-ZERO VACUUM ENERGY DENSITY;

ASTRONOMY;

EID: 0037326330     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20021763     Document Type: Article

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