Gravitational waves in non-singular string cosmologies
Nuclear Physics B, ISSN: 0550-3213, Vol: 607, Issue: 1, Page: 406-428
2001
- 22Citations
- 3Captures
Metric Options: CountsSelecting the 1-year or 3-year option will change the metrics count to percentiles, illustrating how an article or review compares to other articles or reviews within the selected time period in the same journal. Selecting the 1-year option compares the metrics against other articles/reviews that were also published in the same calendar year. Selecting the 3-year option compares the metrics against other articles/reviews that were also published in the same calendar year plus the two years prior.
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.
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 study the evolution of tensor metric fluctuations in a class of non-singular models based on the string effective action, by including in the perturbation equation the higher-derivative and loop corrections needed to regularise the background solutions. We discuss the effects of such higher-order corrections on the final graviton spectrum, and we compare the results of analytical and numerical computations.
Bibliographic Details
http://www.sciencedirect.com/science/article/pii/S0550321301001821; http://dx.doi.org/10.1016/s0550-3213(01)00182-1; http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=0035939576&origin=inward; http://linkinghub.elsevier.com/retrieve/pii/S0550321301001821; http://api.elsevier.com/content/article/PII:S0550321301001821?httpAccept=text/xml; http://api.elsevier.com/content/article/PII:S0550321301001821?httpAccept=text/plain; https://linkinghub.elsevier.com/retrieve/pii/S0550321301001821; https://api.elsevier.com/content/article/PII:S0550321301001821?httpAccept=text/xml; https://api.elsevier.com/content/article/PII:S0550321301001821?httpAccept=text/plain; http://dx.doi.org/10.1016/s0550-3213%2801%2900182-1; https://dx.doi.org/10.1016/s0550-3213%2801%2900182-1
Elsevier BV
Provide Feedback
Have ideas for a new metric? Would you like to see something else here?Let us know