期刊
PHYSICAL REVIEW LETTERS
卷 126, 期 17, 页码 -出版社
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevLett.126.172002
关键词
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资金
- U.S. Department of Energy through the Los Alamos National Laboratory
- National Nuclear Security Administration of U.S. Department of Energy [89233218CNA000001]
- U.S. Department of Energy Office of Science [DE-SC0009919]
- Eccellenza Grant of the Swiss National Science Foundation [PCEFP2_181117]
- RHIC Physics Fellow Program of the RIKEN BNL Research Center
This letter presents a systematic analysis of neutrinoless double beta decay using chiral effective field theory, proposing a method to estimate the numerical value of the exchange coefficient and validating the result by reproducing the charge-independence-breaking contribution to nucleon-nucleon scattering lengths. The central result, derived in dimensional regularization, greatly reduces a crucial uncertainty in the interpretation of searches for neutrinoless double beta decay.
The amplitude for the neutrinoless double beta (0 nu beta beta) decay of the two-neutron system nn -> ppe(-)e(-) constitutes a key building block for nuclear-structure calculations of heavy nuclei employed in large-scale 0 nu beta beta searches. Assuming that the 0 nu beta beta process is mediated by a light-Majorana-neutrino exchange, a systematic analysis in chiral effective field theory shows that already at leading order a contact operator is required to ensure renonnalizability. In this Letter, we develop a method to estimate the numerical value of its coefficient (in analogy to the Cottingham formula for electromagnetic contributions to hadron masses) and validate the result by reproducing the charge-independence-breaking contribution to the nucleon-nucleon scattering lengths. Our central result, while derived in dimensional regularization, is given in terms of the renormalized amplitude A nu(vertical bar p vertical bar,vertical bar p'vertical bar), matching to which will allow one to determine the contact-term contribution in regularization schemes employed in nuclear-structure calculations. Our results thus greatly reduce a crucial uncertainty in the interpretation of searches for 0 nu beta beta decay.
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