Abstract:
A primordial magnetic field may be generated during an inflationary period if conformal invariance is broken. We reexamine and generalize previous results about the magnetic field produced by couplings of the form RnFF. We show that the amplitude of the magnitude field depends strongly on n. For adequate values of n the field produced can serve as a seed for galactic magnetic fields. We also compute the effective interaction between the electromagnetic field and the geometry in the context of scalar QED (with and without classical conformal invariance). In both cases, the ampliutde of the magnetic field is too small to be of astrophysical interest. © 1995 The American Physical Society.
Referencias:
- Parker, E.N., (1979) Cosmical Magnetic Fields, , Clarendon, Oxford
- Ya.B. Zel'dovich, A.A. Ruzmaikin, and D.D. Sokoloff, Magnetic Fields in Astrophysics (Gordon and Breach, New York, 1983); Harrison, E.R., (1973) Phys. Rev. D, 30, p. 188
- Turner, M.S., Widrow, L.M., (1987) Phys. Rev. D, 37, p. 2743
- Ratra, B., (1991), Caltech; Ratra, B., (1992) Astrophys. J., 391, p. L1,
- Gasperini, M., Giovannini, M., Veneziano, G., (1995) Phys. Rev. Lett., 75, p. 3796
- Dolgov, A.D., (1993) Phys. Rev. D, 48, p. 2499
- Drummond, I.T., Hathrell, S.J., (1980) Phys. Rev. D, 22, p. 343
- DeWitt, B.S., (1965) Dynamical Theory of Groups and Fields, , Gordon and Breach, New York
- Cai, Y., (1987) Nucl. Phys., 287 B, p. 279. , and C. N ' u nez
- Kostelecky, V.A., Potting, R., Samuel, S., (1992) Proceedings of the 1991 Joint International Lepton Photon Symposium and Europhysics Conference on High Energy Physics, Geneva, Switzerland, 1991, , edited by, S. Hegarty, K. Potter, E. Quercigh, World Scientific, Singapore
- Parker, L., Toms, D.J., (1985) Phys. Rev. D, 31, p. 953
- Birrell, N.D., Davies, P.C.W, (1982) Quantum Fields in Curved Space, , Cambridge University Press, Cambridge, England
- Barvinsky, A.O., Vilkovisky, G.A., (1985) Phys. Rep., 119, p. 1
- Jack, I., Parker, L., (1985) Phys. Rev. D, 31, p. 2439
- Calzetta, E., Jack, I., Parker, L., (1986) Phys. Rev. D, 33, p. 953
- Dolgov, A.D., (1981) Sov. Phys. JETP, 54, p. 223
Citas:
---------- APA ----------
Mazzitelli, F.D. & Spedalieri, F.M.
(1995)
. Scalar electrodynamics and primordial magnetic fields. Physical Review D, 52(12), 6694-6699.
http://dx.doi.org/10.1103/PhysRevD.52.6694---------- CHICAGO ----------
Mazzitelli, F.D., Spedalieri, F.M.
"Scalar electrodynamics and primordial magnetic fields"
. Physical Review D 52, no. 12
(1995) : 6694-6699.
http://dx.doi.org/10.1103/PhysRevD.52.6694---------- MLA ----------
Mazzitelli, F.D., Spedalieri, F.M.
"Scalar electrodynamics and primordial magnetic fields"
. Physical Review D, vol. 52, no. 12, 1995, pp. 6694-6699.
http://dx.doi.org/10.1103/PhysRevD.52.6694---------- VANCOUVER ----------
Mazzitelli, F.D., Spedalieri, F.M. Scalar electrodynamics and primordial magnetic fields. 1995;52(12):6694-6699.
http://dx.doi.org/10.1103/PhysRevD.52.6694