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Proton Compton Scattering from Linearly Polarized Gamma Rays

  • X. Li
  • , M. W. Ahmed
  • , A. Banu
  • , C. Bartram
  • , B. Crowe
  • , E. J. Downie
  • , M. Emamian
  • , G. Feldman
  • , H. Gao
  • , D. Godagama
  • , H. W. Grießhammer
  • , C. R. Howell
  • , H. J. Karwowski
  • , D. P. Kendellen
  • , M. A. Kovash
  • , K. K.H. Leung
  • , D. M. Markoff
  • , J. A. McGovern
  • , S. Mikhailov
  • , R. E. Pywell
  • M. H. Sikora, J. A. Silano, R. S. Sosa, M. C. Spraker, G. Swift, P. Wallace, H. R. Weller, C. S. Whisnant, Y. K. Wu, Z. W. Zhao

Producción científica: Articlerevisión exhaustiva

7 Citas (Scopus)

Resumen

Differential cross sections for Compton scattering from the proton have been measured at scattering angles of 55°, 90°, and 125° in the laboratory frame using quasimonoenergetic linearly (circularly) polarized photon beams with a weighted mean energy value of 83.4 MeV (81.3 MeV). These measurements were performed at the High Intensity Gamma-Ray Source facility at the Triangle Universities Nuclear Laboratory. The results are compared to previous measurements and are interpreted in the chiral effective field theory framework to extract the electromagnetic dipole polarizabilities of the proton, which gives αE1p=13.8±1.2stat±0.1BSR±0.3theo,βM1p=0.21.2stat±0.1BSR0.3theo in units of 10-4 fm3.

Idioma originalEnglish
Número de artículo132502
PublicaciónPhysical Review Letters
Volumen128
N.º13
DOI
EstadoPublished - abr 1 2022

Nota bibliográfica

Publisher Copyright:
© 2022 American Physical Society.

Financiación

We acknowledge the support of the HIGS accelerator staff for the delivery of high-quality gamma-ray beams and the help with the experimental setup. We acknowledge the contributions of Daniel Phillips to this work. This work is funded in part by the U.S. Department of Energy under Contracts No. DE-FG02-03ER41231, No. DE-FG02-97ER41033, No. DE-FG02-97ER41041, No. DE-FG02-97ER41046, No. DE-FG02-97ER41042, No. DE-SC0005367, No. DE-SC0015393, No. DE-SC0016581, and No. DE-SC0016656, National Science Foundation Grants No. NSF-PHY-0619183, No. NSF-PHY-1309130, and No. NSF-PHY-1714833, UK Science and Technology Facilities Council Grants No. ST/L005794/1 and No. ST/P004423/1, and funds from the Dean of the Columbian College of Arts and Sciences at The George Washington University, and its vice president for research. We acknowledge the financial support of the Natural Sciences and Engineering Research Council of Canada and the support of Eugen Merzbacher Fellowship.

FinanciadoresNúmero del financiador
Columbian College of Arts and Sciences
Natural Sciences and Engineering Research Council of Canada
UK Industrial Decarbonization Research and Innovation Centre
Science and Technology Facilities CouncilST/P004423/1, ST/L005794/1
National Science Foundation Arctic Social Science Program1714833, NSF-PHY-0619183, NSF-PHY-1309130
U.S. Department of EnergyDE-FG02-97ER41046, DE-FG02-97ER41042, DE-FG02-03ER41231, DE-SC0016581, DE-FG02-97ER41033, DE-SC0015393, DE-FG02-97ER41041, DE-SC0016656, DE-SC0005367

    ASJC Scopus subject areas

    • General Physics and Astronomy

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