MG15 - Talk detail |
Participant |
Ivanov, Dimitar | |||||||
Institution |
SISSA - International School for Advanced Studies - Via Bonomea 265 - Trieste - TS - Italy | |||||||
Session |
DE1 |
Accepted |
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Order |
Time |
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Talk |
Oral abstract |
Title |
The Luminosity Distance - Redshift Relation in Cosmologies Beyond FLRW | |||||
Coauthors | ||||||||
Abstract |
Observations from standard candles (such as type Ia supernovae) are usually fitted with a theoretical d_L(z) relation based on simple FLRW cosmology. If one considers departures from such a cosmology, for example due to cosmic structure inhomogeneities or in models beyond the ΛCDM, one needs an improved formula for the luminosity distance. I will show how such a formula can be derived in Conformally FLRW and linearly perturbed FLRW cosmologies. The derivation is based on two different but related approaches - one using the Jacobi map and another using the van Vleck determinant. I will finish by commenting on the application of this formalism to the analysis of present and future data. |
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Pdf file |
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Session |
PT2 |
Accepted |
|
Order |
Time |
|||
Talk |
Oral abstract |
Title |
The Luminosity Distance - Redshift Relation in Cosmologies Beyond FLRW | |||||
Coauthors | ||||||||
Abstract |
Observations from standard candles (such as type Ia supernovae) are usually fitted with a theoretical d_L(z) relation based on simple FLRW cosmology. If one considers departures from such a cosmology, for example due to cosmic structure inhomogeneities or in models beyond the ΛCDM, one needs an improved formula for the luminosity distance. I will show how such a formula can be derived in Conformally FLRW and linearly perturbed FLRW cosmologies. The derivation is based on two different but related approaches - one using the Jacobi map and another using the van Vleck determinant. I will finish by commenting on the application of this formalism to the analysis of present and future data. |
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Pdf file |
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