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Volumn 72, Issue 8, 2004, Pages 1059-1067

Reappraising Einstein's 1909 application of fluctuation theory to Planckian radiation

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EID: 4344593016     PISSN: 00029505     EISSN: None     Source Type: Journal    
DOI: 10.1119/1.1767098     Document Type: Article
Times cited : (7)

References (84)
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    • note
    • For a recent derivation of Eq. (1) as an ensemble average, see W. Greiner, L. Neise, and H. Stöcker, Ref. 4; A. Pais, Subtle is the Lord: The Science and the Life of Albert Einstein (Clarendon, Oxford, 1982), p. 69.
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    • (Springer-Verlag, New York), Chap. 13
    • For a comment to this effect, see R. E. Kelly, "Thermodynamics of blackbody radiation," Am. J. Phys. 49, 714-719 (1981); C. V. Heer, Statistical Mechanics, Kinetic Theory, and Stochastic Processes (Academic, New York, 1972), p. 234. The photon-photon interaction predicted by quantum electrodynamics is too small to be of concern. See J. M. Jauch and F. Rohrlich, The Theory of Photons and Electrons (Springer-Verlag, New York, 1976), Chap. 13.
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    • For an English translation, see the companion volume, translated by A. Beck (Princeton U.P., Princeton), Doc. 61
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    • see W. Greiner, L. Neise, and H. Stöcker., Ref. 4, p. 333
    • Of related interest is that the expansion of the universe causes the spectral distribution of the cosmic background radiation to vary, while maintaining its blackbody character. Such a variation is linked to the gravitational red shift and is not indicative of the radiation being able to thermalize. For a brief discussion, see W. Greiner, L. Neise, and H. Stöcker., Ref. 4, p. 333. For greater detail, see H. Höhl, "A contribution to the thermodynamics of the universe and to 3°K radiation," in Perspectives in Quantum Theory, edited by W. Yourgrau and A. van der Mewe (Dover, New York, 1971), Chap. 8.
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    • A contribution to the thermodynamics of the universe and to 3°K radiation
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    • Of related interest is that the expansion of the universe causes the spectral distribution of the cosmic background radiation to vary, while maintaining its blackbody character. Such a variation is linked to the gravitational red shift and is not indicative of the radiation being able to thermalize. For a brief discussion, see W. Greiner, L. Neise, and H. Stöcker., Ref. 4, p. 333. For greater detail, see H. Höhl, "A contribution to the thermodynamics of the universe and to 3°K radiation," in Perspectives in Quantum Theory, edited by W. Yourgrau and A. van der Mewe (Dover, New York, 1971), Chap. 8.
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    • note
    • In Ref. 2, Einstein refers to A as an increase in momentum and derives Eq. (20) of the present paper. In Ref. l Einstein refers to A as an increase in velocity, though the equation that he derives [Eq. (20) of the present paper] requires that A be viewed as the increase in momentum.
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    • A. Einstein, Ref. 2, p. 386 of the English translation, For a brief account of the reception accorded Einstein's address at the Salzburg Congress of 1909, see A. Hermann, The Genesis of Quantum Theory (1899-1913) (MIT, Cambridge, MA, 1971), Chap. 3, Sec. 7; also the Editorial Note in A. Einstein, The Collected Papers of Albert Einstein, Vol. 2, The Swiss Years: Writings 1900-1909, edited by J. Stachel et al (Princeton U.P., Princeton, 1989), pp. 134-148 (particularly pp. 147-148).
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    • edited by J. Stachel et al. (Princeton U.P., Princeton), Doc. 34
    • A. Einstein, "On the theory of light production and light absorption," Ann. Phys. (Leipzig) 20, 199-206 (1906). Reprinted in A. Einstein, The Collected Papers of Albert Einstein, Vol. 2, The Swiss Years: Writings 19001909, edited by J. Stachel et al. (Princeton U.P., Princeton, 1989), Doc. 34. For an English translation, see the companion volume, The Collected Papers of Albert Einstein, translated by A. Beck (Princeton U.P., Princeton, 1989), Doc. 34 (see particularly p. 196), For a commentary, see M. Jammer, The Conceptual Development of Quantum Mechanics (McGraw-Hill, New York, 1966), pp. 26-27; T. Kuhn, Ref, 30, pp. 184-185.
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    • For an English translation, translated by A. Beck (Princeton U.P., Princeton), Doc. 34 (see particularly p. 196)
    • A. Einstein, "On the theory of light production and light absorption," Ann. Phys. (Leipzig) 20, 199-206 (1906). Reprinted in A. Einstein, The Collected Papers of Albert Einstein, Vol. 2, The Swiss Years: Writings 19001909, edited by J. Stachel et al. (Princeton U.P., Princeton, 1989), Doc. 34. For an English translation, see the companion volume, The Collected Papers of Albert Einstein, translated by A. Beck (Princeton U.P., Princeton, 1989), Doc. 34 (see particularly p. 196), For a commentary, see M. Jammer, The Conceptual Development of Quantum Mechanics (McGraw-Hill, New York, 1966), pp. 26-27; T. Kuhn, Ref, 30, pp. 184-185.
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    • McGraw-Hill, New York
    • A. Einstein, "On the theory of light production and light absorption," Ann. Phys. (Leipzig) 20, 199-206 (1906). Reprinted in A. Einstein, The Collected Papers of Albert Einstein, Vol. 2, The Swiss Years: Writings 19001909, edited by J. Stachel et al. (Princeton U.P., Princeton, 1989), Doc. 34. For an English translation, see the companion volume, The Collected Papers of Albert Einstein, translated by A. Beck (Princeton U.P., Princeton, 1989), Doc. 34 (see particularly p. 196), For a commentary, see M. Jammer, The Conceptual Development of Quantum Mechanics (McGraw-Hill, New York, 1966), pp. 26-27; T. Kuhn, Ref, 30, pp. 184-185.
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    • note
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    • For example, R. E. Sonntag and G. J. van Wylen, Fundamentals of Statistical Thermodynamics (Wiley, New York, 1966), pp. 177-183; S. Tomonaga, Ref. 28, pp. 72-75; H. S. Leff, "Teaching the photon gas in introductory physics," Am. J. Phys. 70, 792-797 (2002).
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    • For example, R. E. Sonntag and G. J. van Wylen, Fundamentals of Statistical Thermodynamics (Wiley, New York, 1966), pp. 177-183; S. Tomonaga, Ref. 28, pp. 72-75; H. S. Leff, "Teaching the photon gas in introductory physics," Am. J. Phys. 70, 792-797 (2002).
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    • Reference 3, Chap, 2
    • Reference 3, Chap, 2; M. V. Klein, Optics (Wiley, New York, 1970), Sec. 6.4; W. Martienssen and E. Spiller, "Coherence and fluctuations in light beams," Am, J. Phys. 32, 919-926 (1964).
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    • Reference 3, Chap, 2; M. V. Klein, Optics (Wiley, New York, 1970), Sec. 6.4; W. Martienssen and E. Spiller, "Coherence and fluctuations in light beams," Am, J. Phys. 32, 919-926 (1964).
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    • note
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    • A. Pais, Ref. 7, pp. 69-70; Ref. 16, p. 69; Ref. 30, pp. 178-179
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    • Reference 6, p. 77 of the English translation
    • Reference 6, p. 77 of the English translation.


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