Phenomenological quark model for baryon magnetic moments and beta decay ratios (GA/GV)

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 66, Issue 3, 2002, Pages 330101-330108

  Franklin, Jerrold ^a  

^a Temple University   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; ATOMIC PARTICLE; CALCULATION; EXCITATION AND STIMULATION; MAGNETIC FIELD; MAGNETISM; MODEL; PHENOMENOLOGY; PREDICTION;

EID: 0036694822     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.66.033010     Document Type: Article

References (30)

1. G. Morpurgo, Physics (Long Island City, N.Y.) 2, 95 (1965); W. Thirring, Acta Phys. Austriaca, Suppl. II, 205 (1965).
2. G. Morpurgo, Physics (Long Island City, N.Y.) 2, 95 (1965); W. Thirring, Acta Phys. Austriaca, Suppl. II, 205 (1965).
3. H.R. Rubinstein, F. Scheck, and R. Socolow, Phys. Rev. 154, 1608 (1967).
4. J. Franklin, Phys. Rev. 172, 1807 (1968).
5. J. Franklin, Phys. Rev. 182, 1607 (1969).
6. Particle Data Group, C. Caso et al., Eur. Phys. J. C 3, 1 (1998).
7. J. Franklin, Phys. Rev. D 20, 1742 (1979); 29, 2648 (1984).
8. J. Franklin, Phys. Rev. D 20, 1742 (1979); 29, 2648 (1984).
9. J. Franklin, Phys. Rev. D 30, 1542 (1984). This paper is referred to as I. There are two misprints in I. Equation (7) should not contain the constant γ which is already included in the definition of the pion emission operator Θ. The right hand side of Eq. (14) should not be divided by nine. Neither of these misprints affected the results because the correct equations were used in all calculations.
10. J. Franklin, Phys. Rev. D 61, 098301 (2000); hep-ph/9807407.
11. Σ- from decuplet states in I that have been corrected here. These errors were small and had negligible effect on the results of I.
12. 2 by less than 1, so we have not bothered to include it in the fit.
13. A.J. Macfarlane and E.C.G. Sudarshan, Nuovo Cimento 31, 1176 (1964); R.H. Dalitz and F. Von Hippel, Phys. Lett. 10, 153 (1964).
14. A.J. Macfarlane and E.C.G. Sudarshan, Nuovo Cimento 31, 1176 (1964); R.H. Dalitz and F. Von Hippel, Phys. Lett. 10, 153 (1964).
15. N. Isgur, Phys. Rev. D 21, 779 (1980); 23, 817(E) (1981).
16. N. Isgur, Phys. Rev. D 21, 779 (1980); 23, 817(E) (1981).
17. J. Franklin, D.B. Lichtenberg, W. Namgung, and D. Carydas, Phys. Rev. D 24, 2910 (1981).
18. G. Karl, Phys. Lett. B 328, 149 (1994); 341, 449(E) (1995).
19. G. Karl, Phys. Lett. B 328, 149 (1994); 341, 449(E) (1995).
20. J. Franklin, Phys. Rev. D 55, 425 (1997).
21. G. Lopez Castro and A. Mariano, Phys. Lett. B 517, 339 (2001).
22. The KTeV experiment at Fermilab reported by Nickolas Solomey in hep-ex/0011024.
23. S. Schadmand, Acta Phys. Pol. B 31, 2431 (2000).
24. L.E. Marcucci et al., Phys. Rev. C 63, 015801 (2001).
25. S.Y. Hsueh et al., Phys. Rev. D 38, 2056 (1988).
26. R.D. Field and R.P. Feynman, Phys. Rev. D 15, 2590 (1977).
27. P. Amaudruz et al., Phys. Rev. Lett. 66, 2712 (1991); Phys. Lett. B 295, 159 (1992); Phys. Lett. B 295, 159 (1992); M. Arneodo et al., Phys. Rev. D 50, R1 (1994).
28. P. Amaudruz et al., Phys. Rev. Lett. 66, 2712 (1991); Phys. Lett. B 295, 159 (1992); Phys. Lett. B 295, 159 (1992); M. Arneodo et al., Phys. Rev. D 50, R1 (1994).
29. P. Amaudruz et al., Phys. Rev. Lett. 66, 2712 (1991); Phys. Lett. B 295, 159 (1992); Phys. Lett. B 295, 159 (1992); M. Arneodo et al., Phys. Rev. D 50, R1 (1994).
30. J.F. Donoghue and B.R. Holstein, Phys. Rev. D 25, 206 (1982).