- Access by Xinjiang University
Baryon magnetic moments in large- chiral perturbation theory: Effects of the decuplet-octet mass difference and flavor symmetry breaking
Phys. Rev. D 89, 034012 – Published 7 February, 2014
DOI: https://doi.org/10.1103/PhysRevD.89.034012
Abstract
The magnetic and transition magnetic moments of the ground-state baryons are computed in heavy baryon chiral perturbation theory in the large- limit, where is the number of colors. SU(3) symmetry breaking is systematically studied twofold: On the one hand, one-loop nonanalytic corrections of orders and are included, with contributions of baryon intermediate states from both flavor octet and flavor decuplet multiplets, assuming degeneracy between baryon states within a given flavor multiplet but nondegeneracy between baryons of different multiplets. On the other hand, perturbative SU(3) symmetry breaking is also analyzed by including all relevant leading-order operators that explicitly break SU(3) at linear order. The resultant expressions are compared with the available experimental data and with other determinations in the context of conventional heavy baryon chiral perturbation theory for three flavors of light quarks and at the physical value . The agreement reached is quite impressive.
See Also
Dirac form factors and electric charge radii of baryons in the combined chiral and expansions
Article Text
References (27)
- S. R. Coleman and S. L. Glashow, Phys. Rev. Lett. 6, 423 (1961).
- S. R. Coleman, Aspects of Symmetry. Selected Erice Lectures (Cambridge University Press, Cambridge, England, 1985).
- E. Jenkins and A. V. Manohar, Phys. Lett. B 255, 558 (1991).
- E. Jenkins and A. V. Manohar, Phys. Lett. B 259, 353 (1991).
- R. F. Dashen, E. Jenkins, and A. V. Manohar, Phys. Rev. D 49, 4713 (1994); R. F. Dashen, E. Jenkins, and A. V. Manohar, ibid. 51, 2489(E) (1995).
- R. F. Dashen, E. Jenkins, and A. V. Manohar, Phys. Rev. D 51, 3697 (1995).
- E. Jenkins, Phys. Rev. D 53, 2625 (1996).
- D. G. Caldi and H. Pagels, Phys. Rev. D 10, 3739 (1974).
- R. Flores-Mendieta, C. P. Hofmann, E. Jenkins, and A. V. Manohar, Ph\ys. Rev. D 62, 034001 (2000).
- R. Flores-Mendieta, Phys. Rev. D 80, 094014 (2009).
- E. Jenkins, M. E. Luke, A. V. Manohar, and M. J. Savage, Phys. Lett. B 302, 482 (1993); 388, 866(E) (1996).
- U.-G. Meissner and S. Steininger, Nucl. Phys. 499B, 349 (1997).
- L. S. Geng, J. M. Camalich, L. Alvarez-Ruso, and M. J. V. Vacas, Phys. Rev. Lett. 101, 222002 (2008).
- L. S. Geng, J. Martin Camalich, and M. J. Vicente Vacas, Phys. Rev. D 80, 034027 (2009).
- D. Arndt and B. C. Tiburzi, Phys. Rev. D 69, 014501 (2004).
- J. Beringer et al. (Particle Data Group Collaboration), Phys. Rev. D 86, 010001 (2012).
- J. Dai, R. F. Dashen, E. Jenkins, and A. V. Manohar, Phys. Rev. D 53, 273 (1996).
- R. Flores-Mendieta, M. A. Hernandez-Ruiz, and C. P. Hofmann, Phys. Rev. D 86, 094041 (2012).
- R. Flores-Mendieta and C. P. Hofmann, Phys. Rev. D 74, 094001 (2006).
- M. A. Luty, J. March-Russell, and M. J. White, Phys. Rev. D 51, 2332 (1995).
- R. F. Lebed and D. R. Martin, Phys. Rev. D 70, 016008 (2004).
- A. Krause, Helv. Phys. Acta 63, 3 (1990).
- E. E. Jenkins, Phys. Rev. D 85, 065007 (2012).
- G. Lopez Castro and A. Mariano, Phys. Lett. B 517, 339 (2001).
- D. Keller et al. (CLAS Collaboration), Phys. Rev. D 83, 072004 (2011).
- D. Keller et al. (CLAS Collaboration), Phys. Rev. D 85, 052004 (2012).
- D. Keller and K. Hicks, Eur. Phys. J. A 49, 53 (2013).