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Contrasting Classical and Quantum Vacuum States in Non-inertial Frames

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Abstract

Classical electron theory with classical electromagnetic zero-point radiation (stochastic electrodynamics) is the classical theory which most closely approximates quantum electrodynamics. Indeed, in inertial frames, there is a general connection between classical field theories with classical zero-point radiation and quantum field theories. However, this connection does not extend to noninertial frames where the time parameter is not a geodesic coordinate. Quantum field theory applies the canonical quantization procedure (depending on the local time coordinate) to a mirror-walled box, and, in general, each non-inertial coordinate frame has its own vacuum state. In particular, there is a distinction between the “Minkowski vacuum” for a box at rest in an inertial frame and a “Rindler vacuum” for an accelerating box which has fixed spatial coordinates in an (accelerating) Rindler frame. In complete contrast, the spectrum of random classical zero-point radiation is based upon symmetry principles of relativistic spacetime; in empty space, the correlation functions depend upon only the geodesic separations (and their coordinate derivatives) between the spacetime points. The behavior of classical zero-point radiation in a noninertial frame is found by tensor transformations and still depends only upon the geodesic separations, now expressed in the non-inertial coordinates. It makes no difference whether a box of classical zero-point radiation is gradually or suddenly set into uniform acceleration; the radiation in the interior retains the same correlation function except for small end-point (Casimir) corrections. Thus in classical theory where zero-point radiation is defined in terms of geodesic separations, there is nothing physically comparable to the quantum distinction between the Minkowski and Rindler vacuum states. It is also noted that relativistic classical systems with internal potential energy must be spatially extended and can not be point systems. The classical analysis gives no grounds for the “heating effects of acceleration through the vacuum” which appear in the literature of quantum field theory. Thus this distinction provides (in principle) an experimental test to distinguish the two theories.

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Notes

  1. For a recent brief review, see [1]. For an extensive review of work before 1996, see [2]. See also, [3].

  2. An anonymous referee for Ref. [8] wrote: “It is also important to note that, in quantum field theory, if a box with totally reflecting walls starts off at rest with no acceleration, and with its interior in the vacuum state, then has its acceleration slowly increased to the final acceleration, its interior will be in the ‘Rindler vacuum’, not the thermal bath. Those boundaries to the box make a huge difference.” A different referee wrote: “So suppose that we now take the mirror to be inertial for t<0, and then to accelerate uniformly for t>0. Then surely the mirror again introduces extra correlations and breaks some of the supposed symmetries of the zero-point radiation. If two such mirrors form a box of size L, then after a proper time L/c has elapsed along either mirror, one would expect even the radiation in the deep interior of the box to be affected by the mirrors motion.”

  3. A typical comment is that of an anonymous referee for Ref. [8], “… (again assuming that the body is small enough so that the gravitational field does not affect it), …”

  4. See, for example, [9]. We are using unrationalized units.

  5. See for example, [14, 15].

  6. See, for example, [16] or [17] or [18].

  7. See, for example, [19] or [20].

  8. See for example, the canonical quantization discussion of [22].

  9. See the recent review by [27].

  10. An anonymous referee for Ref. [8] wrote: “It is important … to realize that the claim that an accelerated observer see a thermal bath is based on the fact that such an observer, carrying a thermometer (which is insensitive in its operation to the presence of a strong gravitational field) will find it reading a temperature. Steaks will cook, eggs will fry.” Later this same referee wrote: “I cannot recommend a paper that denies a quantum field theory direct consequence, namely, that under uniform acceleration a small thermometer will register a temperature. Accelerated enough steaks in Minkowski vacuum will cook, and eggs will fry.”

  11. See Ref. [11], p. 105024-9.

  12. This point of view was not shared by a referee for Ref. [8] who declared, “If there is any disagreement with the standard quantum treatment then this approach is surely wrong.”

References

  1. Boyer, T.H.: Any classical description of nature requires classical electromagnetic zero-point radiation. Am. J. Phys. 79, 1163–1167 (2011)

    Article  ADS  Google Scholar 

  2. de la Pena, L., Cetto, A.M.: The Quantum Dice: An Introduction to Stochastic Electrodynamics. Kluwer, Boston (1996)

    Google Scholar 

  3. Boyer, T.H.: Random electrodynamics: the theory of classical electrodynamics with classical electromagnetic zero-point radiation. Phys. Rev. 11, 790–808 (1975)

    ADS  Google Scholar 

  4. Boyer, T.H.: General connection between random electrodynamics and quantum electrodynamics for free electromagnetic fields and for dipole oscillator systems. Phys. Rev. D 11, 809–830 (1975)

    Article  ADS  Google Scholar 

  5. Marshall, T.W.: Statistical electrodynamics. Proc. Camb. Philol. Soc. 61, 537–546 (1965)

    Article  ADS  MATH  Google Scholar 

  6. Boyer, T.H.: Derivation of the blackbody radiation spectrum without quantum assumptions. Phys. Rev. 182, 1374–11383 (1969)

    Article  ADS  Google Scholar 

  7. Boyer, T.H.: Conformal symmetry of classical electromagnetic zero-point radiation. Found. Phys. 19, 349–365 (1989)

    Article  MathSciNet  ADS  Google Scholar 

  8. Boyer, T.H.: Classical and quantum interpretations regarding thermal behavior in a coordinate frame accelerating through zero-point radiation. arXiv:1011.1426

  9. Goldstein, H.: Classical Mechanics, 2nd edn., pp. 575–578. Addison-Wesley, Reading (1981)

    Google Scholar 

  10. Boyer, T.H.: Classical physics of thermal scalar radiation in two spacetime dimensions. Am. J. Phys. 79, 644–656 (2011)

    Article  ADS  Google Scholar 

  11. Boyer, T.H.: Derivation of the Planck spectrum for relativistic classical scalar radiation from thermal equilibrium in an accelerating frame. Phys. Rev. D 81, 105024 (2010)

    Article  ADS  Google Scholar 

  12. Boyer, T.H.: The blackbody radiation spectrum follows from zero-point radiation and the structure of relativistic spacetime in classical physics. Found. Phys. 42, 595–614 (2012)

    Article  ADS  MATH  Google Scholar 

  13. Boyer, T.H.: Classical statistical thermodynamics and electromagnetic zero-point radiation. Phys. Rev. 186, 1304–1318 (1969)

    Article  ADS  Google Scholar 

  14. Rindler, W.: Essential Relativity: Special, General, and Cosmological, 2nd edn. Springer, New York (1977). pp. 51–59, 156

    MATH  Google Scholar 

  15. Rindler, W.: Kruskal space and the uniformly accelerated frame. Am. J. Phys. 34, 1174–1178 (1966)

    Article  ADS  Google Scholar 

  16. Schutz, B.F.: A First Course in General Relativity. Cambridge, London (1985), p. 150

  17. Hamilton, J.D.: The uniformly accelerated reference frame. Am. J. Phys. 46, 83–89 (1978)

    Article  MathSciNet  ADS  Google Scholar 

  18. Van Meter, J.R., Carlip, S., Hartemann, F.V.: Reflection of plane waves from a uniformly accelerating mirror. Am. J. Phys. 69, 783–787 (2001)

    Article  ADS  Google Scholar 

  19. Greenberg, M.D.: Advanced Engineering Mathematics, 2nd edn. Prentice Hall, Upper Saddle River (1998). Sect. 17.7

    Google Scholar 

  20. Matthews, J., Walker, R.L.: Mathematical Methods of Physics, 2nd edn. Benjamin/Cummins, Reading (1970). pp. 264, 338

    Google Scholar 

  21. Gradshteyn, I.S., Ryzhik, I.M.: Tables of Integrals, Series, and Products, p. 494. Academic Press, New York (1965). \(\int^{\infty}_{0} dxx^{2m} \sin bx/(e^{x}-1)=(-1)^{m}\partial^{2m}/\partial b^{2m} [ (\pi/2)\coth b\pi-(1/2b)]\), (b>0)

    Google Scholar 

  22. Carroll, S.: Spacetime and Geometry: An Introduction to General Relativity, pp. 394–402. Addison-Wesley Longman, Reading (2003)

    Google Scholar 

  23. Fulling, S.A.: Nonuniqueness of canonical field quantization in Riemannian space-time. Phys. Rev. D 7, 2850–2862 (1973)

    Article  ADS  Google Scholar 

  24. Davies, P.C.: Scalar particle production in Schwarzschild and Rindler metrics. J. Phys. A 8, 609–616 (1975)

    Article  ADS  Google Scholar 

  25. Unruh, W.G.: Notes on blackhole evaporation. Phys. Rev. D 14, 870–892 (1976)

    Article  ADS  Google Scholar 

  26. Alsing, P.M., Milonni, P.W.: Simplified derivation of the Hawking-Unruh temperature for an accelerated observer in vacuum. Am. J. Phys. 72, 1524–1529 (2004)

    Article  ADS  Google Scholar 

  27. Crispino, L.C.B., Higuchi, A., Matsas, G.E.A.: The Unruh effect and its applications. Rev. Mod. Phys. 80, 787–838 (2008)

    Article  MathSciNet  ADS  MATH  Google Scholar 

  28. Boyer, T.H.: Thermal effects of acceleration through random classical radiation. Phys. Rev. D 21, 2137–2148 (1980)

    Article  MathSciNet  ADS  Google Scholar 

  29. Boyer, T.H.: Thermal effects of acceleration for a classical dipole oscillator in classical electromagnetic zero-point radiation. Phys. Rev. D 29, 1089–1095 (1984)

    Article  ADS  Google Scholar 

  30. Cole, D.C.: Properties of a classical charged harmonic oscillator accelerated through classical electromagnetic zero-point radiation. Phys. Rev. D 31, 1972–1981 (1985)

    Article  MathSciNet  ADS  Google Scholar 

  31. Boyer, T.H.: Thermal effects of acceleration for a classical spinning magnetic dipole in classical electromagnetic zero-point radiation. Phys. Rev. D 30, 1228–1232 (1984)

    Article  ADS  Google Scholar 

  32. Boyer, T.H.: Example of mass-energy relation: classical hydrogen atom accelerated or supported in a gravitational field. Am. J. Phys. 66, 872–876 (1998)

    Article  ADS  Google Scholar 

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Boyer, T.H. Contrasting Classical and Quantum Vacuum States in Non-inertial Frames. Found Phys 43, 923–947 (2013). https://doi.org/10.1007/s10701-013-9726-4

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