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A quantitative assessment of stochastic electrodynamics
with spin (SEDS): Physical principles and novel applications |
Giancarlo CAVALLERI1,Francesco BARBERO1,Gianfranco BERTAZZI1,Eros CESARONI1,Ernesto TONNI1,Leonardo BOSI2,Gianfranco SPAVIERI3,George T. GILLIES4, |
1.Dipartimento di
Matematica e Fisica, Università Cattolica del Sacro Cuore, via
Musei 41, 25121 Brescia, Italy; 2.Politecnico di
Milano (Polo Regionale di Lecco), Dipartimento di Fisica, piazza L.
da Vinci 32, 20133 Milano, Italy; 3.Centro de Física
Fundamental, Facultad de Ciencias, Universidad de Los Andes, Mérida,
5101 Venezuela; 4.School of Engineering
and Applied Science, University of Virginia, Charlottesville, VA 22904-4746,
USA; |
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Abstract Stochastic electrodynamics (SED) without spin, denoted as pure SED, has been discussed and seriously considered in the literature for several decades because it accounts for important aspects of quantum mechanics (QM). SED is based on the introduction of the nonrenormalized, electromagnetic stochastic zero-point field (ZPF), but neglects the Lorentz force due to the radiation random magnetic field Br. In addition to that rather basic limitation, other drawbacks remain, as well: i) SED fails when there are nonlinear forces; ii) it is not possible to derive the Schrödinger equation in general; iii) it predicts broad spectra for rarefied gases instead of the observed narrow spectral lines; iv) it does not explain double-slit electron diffraction patterns. We show in this short review that all of those drawbacks, and mainly the first most basic one, can be overcome in principle by introducing spin into stochastic electrodynamics (SEDS). Moreover, this modification of the theory also explains four observed effects that are otherwise so far unexplainable by QED, i.e., 1) the physical origin of the ZPF, and its natural upper cutoff; 2) an anomaly in experimental studies of the neutrino rest mass; 3) the origin and quantitative treatment of 1/f noise; and 4) the high-energy tail (~ 1021 eV) of cosmic rays. We review the theoretical and experimental situation regarding these things and go on to propose a double-slit electron diffraction experiment that is aimed at discriminating between QM and SEDS. We show that, in the context of this experiment, for the case of an electron beam focused on just one of the slits, no interference pattern due to the other slit is predicted by QM, while this is not the case for SEDS. A second experiment that could discriminate between QED and SEDS regards a transversely large electron beam including both slits obtained in an insulating wall, where the ZPF is reduced but not vanished. The interference pattern according to SEDS should be somewhat modified with respect to QED’s.
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Keywords
quantum mechanics
Aharonov–Bohm effect
spin
electrodynamics
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Issue Date: 05 March 2010
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|
|
R. P. Feynman, QED: The Strange Theory of Light and Matter, 7th Ed., Princeton: Princeton UniversityPress, 1988: 9
|
|
L. Bosi and G. Cavalleri, Nuovo Cimento B, 2002, 117: 243
|
|
G. Cavalleri and L. Bosi, Phys. Stat. Sol. (c), 2007, 4: 1230
doi: 10.1002/pssc.200673705
|
|
G. Cavalleri, E. Tonni, L. Bosi, and G. Spavieri, Fluct. Noise Lett., 2007, 7: L193
|
|
E. Nelson, Phys. Rev., 1966, 150(4): 1079
doi: 10.1103/PhysRev.150.1079
|
|
J. G. Gilson, Proc. Cambridge Philos. Soc., 1968, 74(4): 1061
doi: 10.1017/S0305004100043826
|
|
A. F. Kracklauer, Phys. Rev. D, 1974, 10(4): 1358
doi: 10.1103/PhysRevD.10.1358
|
|
G. Cavalleri, Phys. Rev. D, 1981, 23(2): 363
doi: 10.1103/PhysRevD.23.363
|
|
L. De la Pe?a-Auerbach and A. M. Cetto, Found. Phys., 1975, 5 (2): 355
|
|
A. Carati and L. Galgani, Phys. Rev. E, 2000, 61(5): 4791
doi: 10.1103/PhysRevE.61.4791
|
|
G. Cavalleri and E. Cesaroni, Phys. Rev. E, 2003, 68: 028101
doi: 10.1103/PhysRevE.68.028101
|
|
A. Carati and L. Galgani, Phys. Rev. E, 2003, 68: 028102
doi: 10.1103/PhysRevE.68.028102
|
|
A. Carati, L. Galgani, and B. Pozzi, Phys. Rev. Lett., 2003, 90: 010601
doi: 10.1103/PhysRevLett.90.010601
|
|
For a more readable derivation, see: T. H. Boyer, Phys. Rev., 1969, 182: 1374
doi: 10.1103/PhysRev.182.1374
|
|
T. H. Boyer, Phys. Rev. D, 1975, 11: 790
doi: 10.1103/PhysRevD.11.790
|
|
G. Cavalleri, E. Tonni, C. Bernasconi, and P. Di Sia, Nuovo Cimento B, 2001, 116: 1353
|
|
G. Cavalleri, F. Barbero, E. Tonni, D. Molteni, G. Bottoni, and S. Lacchin, in: Proc. of X Int. Conf., Physical Interpretations of Relativity Theory, London, September, 8―112006, edited by M. C. Duffy, University of Sunderland,PD Publications, Liverpool, Great Britain, 2008, Vol. I (in press)
|
|
T. W. Marshall and P. Claverie, J. Math. Phys., 1980, 21: 1819
doi: 10.1063/1.524635
|
|
A. Rueda and G. Cavalleri, Nuovo Cimento C, 1983, 6: 239
|
|
H. E. Puthoff, Phys. Rev. D, 1987, 35: 3266
doi: 10.1103/PhysRevD.35.3266
|
|
M. Surdin, P. Braffort, and A. Taroni, Nature, 1966, 210(5034): 405
doi: 10.1038/210405a0
|
|
E. Santos, Nuovo Cimento B, 1974, 19(1): 57
doi: 10.1007/BF02749757
|
|
L. De la Pe?a-Auerbach and A. M. Cetto, J. Math. Phys., 1979, 20(3): 469
|
|
T. H. Boyer, Phys. Rev. A, 1980, 21: 66
doi: 10.1103/PhysRevA.21.66
|
|
T. H. Boyer, Phys. Rev. D, 1984, 29: 1089
doi: 10.1103/PhysRevD.29.1089
|
|
A. Rueda, Nuovo Cimento A, 1978, 48: 155
doi: 10.1007/BF02799672
|
|
A. Rueda, Phys. Rev. A, 1981, 23: 2020
doi: 10.1103/PhysRevA.23.2020
|
|
L. De la Pe?a-Auerbach, Stochastic Electrodynamics: its development, presentsituation, and perspectives, in: Stochastic Processes Applied to Physicsand other Related Fields, edited by G. Gomez, S. M. Moore, A. M. Rodriguez-Vargas, and A. Rueda, World Scientific, 1983: 428―649. The criticism to Boyer's 1969 paper [14], is found in: L.De la Pe?a-Auerbach and A. M. Cetto, The Quantum Dice, Kluwer,1996, Chap. 5, Sec. 5.2: 1476
|
|
B. Haisch, A. Rueda, and H. E. Puthoff, Phys. Rev. A, 1994, 49: 678
doi: 10.1103/PhysRevA.49.678
|
|
A. Rueda, B. Haisch, and D. C. Cole, Astrophys. J., 1995, 445: 7
doi: 10.1086/175667
|
|
D. C. Cole, A. Rueda, and K. Danley, Phys. Rev. A, 2001, 63: 054101
doi: 10.1103/PhysRevA.63.054101
|
|
A. Rueda and B. Haisch, Ann. Phys. (Leipzig), 2005, 14: 479
doi: 10.1002/andp.200510147
|
|
Y. S. Levin, Phys. Rev. A, 2009, 79: 012114
doi: 10.1103/PhysRevA.79.012114
|
|
L. Pesquera and P. Claverie, J. Math. Phys., 1982, 23: 1315
doi: 10.1063/1.525516
|
|
A. O. Barut and N. Zanghi, Phys. Rev. Lett., 1984, 52: 2009
doi: 10.1103/PhysRevLett.52.2009
|
|
G. Cavalleri, Nuovo Cimento B, 1997, 112: 1193
|
|
I. Pitowsky, Phys. Rev Lett., 1982, 48: 1299
doi: 10.1103/PhysRevLett.48.1299
|
|
D. Z. Albert and R. Galchen, Was Einstein Wrong?: A QuantumThreat to Special Relativity, in: ScientificAmerican Magazine, March2009
|
|
A. Aspect, J. Dalibard, and G. Roger, Phys. Rev. Lett., 1982, 49: 1804
doi: 10.1103/PhysRevLett.49.1804
|
|
G. Cavalleri, E. Cesaroni, and E. Tonni, in: Recent advances in Relativity Theory2: material interpretations, edited by M. C. Duffy and M. Wegener, Palm Harbor, Florida(USA): Hadronic Press, 2001, Vol. 2: 19
|
|
G. Cavalleri, Lett. Nuovo Cimento, 1985, 43: 285
doi: 10.1007/BF02751922
|
|
G. Cavalleri and G. Spavieri, Nuovo Cimento B, 1986, 95: 194
doi: 10.1007/BF02749010
|
|
J. Maddox, Nature (London), 1987, 325: 385
doi: 10.1038/325385a0
|
|
G. Cavalleri and G. Mauri, Phys. Rev. B, 1990, 41: 6751
doi: 10.1103/PhysRevB.41.6751
|
|
G. Cavalleri and A. Zecca, Phys. Rev. B, 1991, 43: 3223
doi: 10.1103/PhysRevB.43.3223
|
|
A. Zecca and G. Cavalleri, Nuovo Cimento B, 1997, 112: 1
|
|
G. Cavalleri and E. Tonni, in: The Foundation of QuantumMechanics – Historical Analysis and Open Questions –Lecce 1998, edited by C. Garola and A. Rossi, World Scientific Publ., 2000: 111
|
|
A. Tonomura, N. Osakabe, T. Matsuda, T. Kawasaki, and J. Endo, Phys. Rev. Lett., 1986, 56: 792
doi: 10.1103/PhysRevLett.56.792
|
|
N. Osakabe, et al, Phys. Rev. A, 1986, 34: 815
doi: 10.1103/PhysRevA.34.815
|
|
A. Tonomura, et al., Am. J. Phys., 1989, 57: 117
doi: 10.1119/1.16104
|
|
Y. Aharonov and D. Bohm, Phys. Rev., 1959, 115: 48
doi: 10.1103/PhysRev.115.485
|
|
Y. Aharonov and A. Casher, Phys. Rev. Lett., 1984, 53: 319
doi: 10.1103/PhysRevLett.53.319
|
|
G. Spavieri, Phys. Rev. Lett., 1998, 81: 1533
doi: 10.1103/PhysRevLett.81.1533
|
|
G. Spavieri, Phys. Rev. A, 1999, 59: 3194
doi: 10.1103/PhysRevA.59.3194
|
|
X. G. He and B. H. J. McKellar, Phys. Rev. A, 1993, 47: 3424
doi: 10.1103/PhysRevA.47.3424
|
|
M. Wilkens, Phys. Rev. A, 1994, 49: 570
doi: 10.1103/PhysRevA.49.570
|
|
M. Wilkens, Phys. Rev. Lett., 1994, 72: 5
doi: 10.1103/PhysRevLett.72.5
|
|
J. Anandan, Phys. Rev. Lett., 2000, 85: 1354
doi: 10.1103/PhysRevLett.85.1354
|
|
V. M. Tkachuk, Phys. Rev. A, 2000, 62: 052112―1
doi: 10.1103/PhysRevA.62.052112
|
|
G. Spavieri, Phys. Rev. Lett., 1999, 82: 3932
doi: 10.1103/PhysRevLett.82.3932
|
|
G. Spavieri, Phys. Lett. A, 2003, 310: 13
doi: 10.1016/S0375-9601(03)00203-2
|
|
G. Spavieri, Eur. Phys. J. D, 2006, 39: 157
doi: 10.1140/epjd/e2006-00089-y
|
|
T. H. Boyer, Phys. Rev. A, 1987, 36: 5083
doi: 10.1103/PhysRevA.36.5083
|
|
T. H. Boyer, Nuovo Cimento B, 1987, 100: 685
|
|
G. Spavieri and G. Cavalleri, Europhys. Lett., 1992, 18: 301
doi: 10.1209/0295-5075/18/4/004
|
|
G. Spavieri, Eur. J. Phys. D, 2006, 37: 327
doi: 10.1140/epjd/e2005-00328-9
|
|
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