Probabitlity for Primordial Black holes Pair in 1/R Gravity

dc.contributor.authorPaul, Dilip
dc.contributor.authorPaul, B. C.
dc.date.accessioned2012-03-06T10:03:10Z
dc.date.available2012-03-06T10:03:10Z
dc.date.issued2005-08-01
dc.description.abstractThe probability for quantum creation of an inflationary universe with a pair of black holes in 1/R - gravitational theory has been studied. Considering a gravitational action which includes a cosmological constant (Λ) in addition to δ R−1 term, the probability has been evaluated in a semiclassical approximation with Hartle-Hawking boundary condition. We obtain instanton solutions determined by the parameters δ and Λ satisfying the constraint δ ≤ 4Λ23 . However, we note that two different classes of instanton solutions exists in the region 0 < δ < 4Λ23 . The probabilities of creation of such configurations are evaluated. It is found that the probability of creation of a universe with a pair of black holes is strongly suppressed with a positive cosmological constant except in one case when 0 < δ < Λ2. It is also found that gravitational instanton solution is permitted even with Λ = 0 but one has to consider δ < 0. However, in the later case a universe with a pair of black holes is less probable.en_US
dc.identifier.urihttp://hdl.handle.net/11007/723
dc.language.isoenen_US
dc.relation.ispartofseriesIUCAA Preprint;39/05
dc.subjectBlack Holesen_US
dc.titleProbabitlity for Primordial Black holes Pair in 1/R Gravityen_US
dc.typeArticleen_US

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