Black holes in accelerated universe
International Journal of Theoretical Physics, ISSN: 0020-7748, Vol: 49, Issue: 8, Page: 1706-1711
2010
- 4Citations
- 5Captures
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Example: if you select the 1-year option for an article published in 2019 and a metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019. If you select the 3-year option for the same article published in 2019 and the metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019, 2018 and 2017.
Citation Benchmarking is provided by Scopus and SciVal and is different from the metrics context provided by PlumX Metrics.
Article Description
We have analyzed the evolution of mass of a stationary black hole in the standard FRW cosmological model. The evolution is determined specifically about the time of transition from the earlier matter to the later exotic dark energy dominated universe. It turns out that the accretion rate of matter on the black hole of mass was approximately O(10) higher than the accretion rate of exotic dark energy at the time of transition. © 2010 Springer Science+Business Media, LLC.
Bibliographic Details
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=77955280081&origin=inward; http://dx.doi.org/10.1007/s10773-010-0350-1; http://link.springer.com/10.1007/s10773-010-0350-1; http://link.springer.com/content/pdf/10.1007/s10773-010-0350-1; http://link.springer.com/content/pdf/10.1007/s10773-010-0350-1.pdf; http://link.springer.com/article/10.1007/s10773-010-0350-1/fulltext.html; http://www.springerlink.com/index/10.1007/s10773-010-0350-1; http://www.springerlink.com/index/pdf/10.1007/s10773-010-0350-1; https://dx.doi.org/10.1007/s10773-010-0350-1; https://link.springer.com/article/10.1007/s10773-010-0350-1
Springer Science and Business Media LLC
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