Ir directamente a la navegación principal Ir directamente a la búsqueda Ir directamente al contenido principal

Detecting the flavor content of the vacuum using the Dirac operator spectrum

Producción científica: Articlerevisión exhaustiva

2 Citas (Scopus)

Resumen

We compute the overlap Dirac spectrum on three gauge ensembles generated using 2+1-flavor domain wall fermions. The three ensembles have different lattice spacings, and two of them have quark masses tuned to the physical point. The spectral density is determined up to λ∼100 MeV with subpercentage statistical uncertainty. We find that the density is close to a constant below λ∼20 MeV as predicted by chiral perturbative theory (χPT) and then increases linearly due to the strange quark mass. By fitting to the next-to-leading order χPT form and using the nonperturbative renormalization using the regularization independent momentum subtraction scheme, the SU(2) (keeping the strange quark mass at the physical point) and SU(3) chiral condensates at MS¯ 2 GeV are determined to be ς=(265.4(0.5)(4.2) MeV)3 and ς0=(234.3(0.5)(25.8) MeV)3, respectively. The pion decay constants are also determined to be F=84.1(1.9)(8.0) and F0=58.6(0.5)(10.0) MeV. The systematic errors are carefully estimated including the effects of fitting ranges and the uncertainty of low-energy constant L6. We also show that one can resolve the sea flavor content of the sea quarks and constrain their masses with ∼10%-20% statistical uncertainties using the Dirac spectral density.

Idioma originalEnglish
Número de artículo094513
PublicaciónPhysical Review D
Volumen110
N.º9
DOI
EstadoPublished - nov 1 2024

Nota bibliográfica

Publisher Copyright:
© 2024 authors.

Financiación

This work is partially supported by the Guangdong Major Project of Basic and Applied Basic Research Grant No. 2020B0301030008. J.L. is supported by the Natural Science Foundation of China under Grants No. 12175073 and No. 12222503 and the Natural Science Foundation of Basic and Applied Basic Research of Guangdong Province under Grant No. 2023A1515012712. A.A. is supported in part by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics under Grant No. DE-FG02-95ER40907. Y.-J.B. is supported in part by the National Natural Science Foundation of China (NNSFC) under Grant No. 12075253. T.D. and K.-F.L. are supported by the U.S. DOE Grant No. DE-SC0013065 and DOE Grant No. DE-SC0023646 which is within the framework of the Quark-Gluon Tomography (QGT) Topical Collaboration. Y.-B. Y is also supported by the NSFC Grants No. 12293060, No. 12293062, and No. 12047503, the Strategic Priority Research Program of Chinese Academy of Sciences, Grants No. XDB34030303 and No. YSBR-101. The numerical calculations were carried out on the ORISE Supercomputer, HPC Cluster of ITP-CAS, and the Southern Nuclear Science Computing Center (SNSC). This work also used Stampede time under the Extreme Science and Engineering Discovery Environment (XSEDE), which is supported by National Science Foundation Grant No. ACI1053575. We also used resources on Frontera at Texas Advanced Computing Center (TACC). We also thank the National Energy Research Scientific Computing Center (NERSC) for providing HPC resources that have contributed to the research results reported within this paper. We thank the RBC and UKQCD Collaborations for providing us their DWF gauge configurations. The calculations were performed using the GWU code through the HIP programming model . This work is partially supported by the Guangdong Major Project of Basic and Applied Basic Research Grant No. 2020B0301030008. J. L. is supported by the Natural Science Foundation of China under Grants No. 12175073 and No. 12222503 and the Natural Science Foundation of Basic and Applied Basic Research of Guangdong Province under Grant No. 2023A1515012712. A. A. is supported in part by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics under Grant No. DE-FG02-95ER40907. Y.-J. B. is supported in part by the National Natural Science Foundation of China (NNSFC) under Grant No. 12075253. T. D. and K.-F. L. are supported by the U.S. DOE Grant No. DE-SC0013065 and DOE Grant No. DE-SC0023646 which is within the framework of the Quark-Gluon Tomography (QGT) Topical Collaboration. Y.-B. Y is also supported by the NSFC Grants No. 12293060, No. 12293062, and No. 12047503, the Strategic Priority Research Program of Chinese Academy of Sciences, Grants No. XDB34030303 and No. YSBR-101. The numerical calculations were carried out on the ORISE Supercomputer, HPC Cluster of ITP-CAS, and the Southern Nuclear Science Computing Center (SNSC). This work also used Stampede time under the Extreme Science and Engineering Discovery Environment (XSEDE), which is supported by National Science Foundation Grant No. ACI1053575. We also used resources on Frontera at Texas Advanced Computing Center (TACC). We also thank the National Energy Research Scientific Computing Center (NERSC) for providing HPC resources that have contributed to the research results reported within this paper.

FinanciadoresNúmero del financiador
ITP-CAS
Southern Nuclear Science Computing Center
National Energy Research Scientific Computing Center
Office of Science Programs
National Natural Science Foundation of China (NSFC)12175073, 12293060, 12047503, 12075253, 12222503, 12293062
Guangdong Major Project of Basic and Applied Basic Research2020B0301030008
National Science Foundation Arctic Social Science ProgramACI1053575
Institute for Nuclear PhysicsDE-FG02-95ER40907
U.S. Department of Energy EPSCoRDE-SC0023646, DE-SC0013065
Natural Science Foundation of Basic and Applied Basic Research of Guangdong Province2023A1515012712
Chinese Academy of SciencesXDB34030303, YSBR-101

    ASJC Scopus subject areas

    • Nuclear and High Energy Physics

    Huella

    Profundice en los temas de investigación de 'Detecting the flavor content of the vacuum using the Dirac operator spectrum'. En conjunto forman una huella única.

    Citar esto