Shape and pairing fluctuation effects on neutrinoless double beta decay nuclear matrix elements
Physical Review Letters, ISSN: 0031-9007, Vol: 111, Issue: 14, Page: 142501
2013
- 140Citations
- 33Captures
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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.
Metrics Details
- Citations140
- Citation Indexes140
- 140
- CrossRef130
- Captures33
- Readers33
- 33
Article Description
Nuclear matrix elements (NME) for the most promising candidates to detect neutrinoless double beta decay have been computed with energy density functional methods including deformation and pairing fluctuations explicitly on the same footing. The method preserves particle number and angular momentum symmetries and can be applied to any decay without additional fine tunings. The finite range density dependent Gogny force is used in the calculations. An increase of 10%-40% in the NME with respect to the ones found without the inclusion of pairing fluctuations is obtained, reducing the predicted half-lives of these isotopes. © 2013 American Physical Society.
Bibliographic Details
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=84885012160&origin=inward; http://dx.doi.org/10.1103/physrevlett.111.142501; http://www.ncbi.nlm.nih.gov/pubmed/24138234; https://link.aps.org/doi/10.1103/PhysRevLett.111.142501; http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevLett.111.142501/fulltext; http://link.aps.org/article/10.1103/PhysRevLett.111.142501; http://link.aps.org/doi/10.1103/PhysRevLett.111.142501; http://journals.aps.org/prl/abstract/10.1103/PhysRevLett.111.142501
American Physical Society (APS)
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