Abstract
The unorthodox idea that the gravitational constant G varies slowly in time arose in the late 1930s in the context of a cosmological theory proposed by the English physicist Paul Dirac. The idea was received coolly, not only because it led to a much too small age of the universe but also because it contradicted the general theory of relativity and, on the top of that, was thought to be untestable. However, Dirac’s idea was taken up and further developed by Pascual Jordan in Germany and after World War II it slowly began to attract attention among physicists and astronomers. In 1948 the hypothesis of varying gravity made its first connection to the earth sciences in the form of an attempt, made by Edward Teller, to test the hypothesis by means of a paleoclimatic argument. The test was inconclusive and was initially ignored by the earth scientists.
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Notes
- 1.
On pre-relativistic conceptions of the gravitational law and its associated constant, see Will (1987), Ducheyne (2011), and Uzan and Lehoucq (2005), pp. 253–261. A detailed account of experiments on gravitation until the 1890s is given in Mackenzie (1900). References to the literature can be found in these sources.
- 2.
For details on Cavendish and his experiment, see Jungnickel and McCormmach (1999), pp. 440–460.
- 3.
Boys (1894), p. 330.
- 4.
- 5.
Davis (1904). For Zöllner’s number, see Kragh (2012). Weyl first discussed the number 1040 in 1919 and Eddington in 1923.
- 6.
Poynting (1920), p. 643. See also Ducheyne (2011), p. 2011.
- 7.
- 8.
- 9.
Dirac (1938) referred to the “Fundamental Principle.” He first spoke of the Large Numbers Hypothesis in a talk given in 1972. See Dirac (1973a), p. 46. Pascual Jordan always referred to “Dirac’s principle.” For more details on the history of the principle and Dirac’s cosmology, see Kragh (1990), pp. 223–246 and also Barrow and Tipler (1986). Many of Dirac’s arguments concerning the nature and use of the LNH were questionable and based on somewhat arbitrary assumptions. See, for example, Klee (2002) for an interesting critical review. However, from the point of view of the present book this is less relevant.
- 10.
Dirac (1939), p. 128.
- 11.
Dirac (1938), p. 204.
- 12.
Sambursky (1937).
- 13.
Gamow to the American geophysicist Philip H. Abelson, 1 September 1967, reproduced in Gamow (1967b), p. 767. On 2 January 1937 Dirac married Margit Wigner Balasz, the sister of the Hungarian-American physicist Eugene Wigner.
- 14.
The leading geophysicist Harold Jeffreys was aware of Dirac’s hypothesis as early as June 1937, when he commented on the hypothetical-deductive methodology of Dirac, Milne and Eddington (see Nature 141: 1004–1006). However, neither at this nor at later occasions did he mention the G(t) hypothesis and its possible geological consequences.
- 15.
- 16.
Eddington (1939), p. 234.
- 17.
- 18.
Kothari (1938).
- 19.
Zwicky (1939), p. 733.
- 20.
Smith (1978).
- 21.
Solomon (1938). Solomon, a Jew and a communist, was active in the French resistance movement during the early years of World War II. He was executed by the Germans in 1942.
- 22.
Goldberg (1992), p. 95. Goldberg was a leading physicist in the Aeronautical Research Laboratories (ARL) established in 1955 by the U.S. Air Force. For Jordan and ARL, see Sect. 2.6. Jordan was not invited to participate in the 1958 Solvay Congress on gravitation and cosmology. One may speculate that one of the reasons was that his past as a Nazi was not easily forgotten in formerly occupied Belgium.
- 23.
Jordan (1952), p. 137.
- 24.
Jordan (1961b), p. 2.
- 25.
- 26.
- 27.
- 28.
As expressed by Singh (1970), p. 233, in Jordan’s theory stars came “literally out of the blue like Athena leaping forth from Zeus’s brain mature and in complete armour.” On the request of his former professor Max Born, Jordan wrote a summary article in English of his work in cosmology and astrophysics. See Jordan (1949) and also the critical review of Jordan’s theory in North (1965), pp. 205–208.
- 29.
Bondi (1952), p. 164.
- 30.
Jordan (1944), p. 190.
- 31.
“The construction erected by Pascual Jordan is of undeniable elegance, and at any rate suggests a simple and brilliant interpretation of the expansion.” Couderc (1952), p. 225.
- 32.
Haas (1936). Arthur Erich Haas was at the time professor of physics at Notre Dame University in Indiana. An account of his work in speculative cosmology can be found in Kragh (2004), pp. 189–194.
- 33.
- 34.
Teller (1972), Tryon (1973), Carey (1978), Sciama (1953).
- 35.
ten Bruggencate (1948), which originally appeared in the proceedings of the Göttingen Academy in 1945.
- 36.
Jordan (1938). As mentioned, in the same year Solomon suggested a similar idea.
- 37.
Pauli (1936), p. 76; see also Jordan (1944), p. 186.
- 38.
Houtermans and Jordan (1946), Jordan (1947a), p. 20. Together with the British physicist Robert Atkinson, in 1929 Houtermans pioneered quantum-mechanical nuclear astrophysics. See Kragh (1996), pp. 85–87. After World War II he specialized in geophysics and meteoritics, including radiometric dating methods. In 1953 he estimated the age of the Earth to be 4.5 billion years. For Houtermans’ work and eventful life, see Amaldi (2012).
- 39.
Hönl (1949). See also Dehm (1949).
- 40.
Jordan (1969b), pp. 254–255. See also Jordan et al. (1964), p. 505.
- 41.
See Aldrich et al. (1958). This was possibly the first scientific conference ever specifically devoted to the relationship between cosmology and geology.
- 42.
Kanasewich and Savage (1963).
- 43.
- 44.
According to Nye (2004), p. 17. See also Jordan (1955), pp. 271–272.
- 45.
Blackett (1939).
- 46.
Blackett (1941), p. 213.
- 47.
Jordan (1944).
- 48.
- 49.
Milne (1938).
- 50.
- 51.
Online as http://www.fdavidpeat.com/interviews/dirac.htm.The interview is published in Buckley and Peat (1979).
- 52.
Dirac (1978c), p. 8.
- 53.
- 54.
Haldane (1945b), p. 140.
- 55.
Page (1948), p. 23.
- 56.
Haldane’s theory was critically reviewed by Lemaître and also by the philosopher Robert Cohen. See references in Kragh (2004), p. 225. See also Stanley-Jones (1949). Today the theory is forgotten, and perhaps justly so. It is briefly mentioned in Brush (2001), p. 164.
- 57.
- 58.
Martin Schwarzschild (1912–1997) was the son of the famous German astronomer Karl Schwarzschild (1873–1916). After studies in mathematics and astronomy in Göttingen and Berlin, in 1937 he moved to the United States where he obtained a position at Columbia University and in 1942 became a U.S. citizen. In 1947 he accepted a position at Princeton University.
- 59.
Teller (1948).
- 60.
In his extensive memoirs Teller did not even mention his 1948 excursion into cosmology and paleoclimatology. See Teller and Shoolery (2001).
- 61.
Couderc (1952), p. 98.
- 62.
E.g., Gamow (1949), p. 21, and Omer (1949), p. 166. See also Schatzmann (1966), p. 219, originally published 1957 as Origine et Évolution des Mondes.
- 63.
ter Haar (1950), p. 131.
- 64.
Jordan (1955), p. 235.
- 65.
Jordan (1962b), p. 285. See also Dyson (1972), according to whom S ~ G 9.7 or S ~ t −9.7. As mentioned in Sect. 2.3, ten Bruggencate (1948) was probably the first to consider the effect of the G(t) hypothesis on the Sun’s luminosity.
- 66.
Jordan (1964), p. 114.
- 67.
On the change in the cosmic time scale, see Kragh (1996), pp. 271–276.
- 68.
- 69.
Sandage (1958), p. 525.
- 70.
Pochoda and Schwarzschild (1964), p. 587.
- 71.
- 72.
Gamow (1967c). Other problems in solar nucleosynthesis based on a decreasing gravitational constant were pointed out in Ezer and Cameron (1966).
- 73.
See also Dicke (1962a), which refers to Öpik’s paper of 1961 as “privately circulated.” Fairbridge was at the time a supporter of the hypothesis of a slowly expanding Earth, which was sometimes justified in terms of a decreasing gravitational constant. However, Fairbridge did not accept the Dirac–Jordan hypothesis of G(t). We shall return to Fairbridge in Sect. 3.6.
- 74.
Öpik (1965), p. 292.
- 75.
- 76.
According to Peebles et al. (2009), p. 38.
- 77.
- 78.
- 79.
- 80.
Gamow (1967a), p. 759. It should be noted that the geological periods and the times in the past associated with them have changed considerably during the twentieth century. For example, the “Cambrian” did not have a fixed meaning across the century. Gamow apparently associated the Cambrian with Teller’s period 200–300 million years ago, but according to Holmes’ revised time scale of 1960 the Cambrian ended about 500 million years ago. The presently accepted time for the end of the Cambrian period and the beginning of the Ordovician is 485 million years ago.
- 81.
- 82.
- 83.
Dirac (1982), p. 88.
- 84.
Teller (1972).
- 85.
- 86.
- 87.
Dyson (1972).
- 88.
- 89.
The first scalar–tensor gravitational theory was published in 1941 by the Swiss mathematician Willy Scherrer at the University of Bern. For the origins and early development of scalar–tensor theories, see Goenner (2012).
- 90.
- 91.
- 92.
Ellis (2009), p. 2180.
- 93.
Schücking (2000), p. vi.
- 94.
The ARL reports are listed in Goldberg (1992). One of Jordan’s reports contained a detailed review of geophysical and astronomical aspects related to Dirac’s hypothesis. See Jordan (1961b), a copy of which is located at the Niels Bohr Institute, Copenhagen.
- 95.
Jordan (1948). “Kaluza–Klein” refers to the German mathematician Theodor Kaluza and the Swedish physicist Oskar Klein. While Kaluza’s unification comprised gravitation and electrodynamics, Klein’s theory also included the quantum domain.
- 96.
Bergmann (1948), p. 255. The title of Jordan’s unpublished paper was “Gravitationstheorie mit veränderlicher Gravitationszahl” (Gravitation theory with variable gravitational constant). Bergmann was sceptical with regard to Jordan’s theory because the extra scalar variable caused an embarrass de richesse, as he expressed it.
- 97.
Jordan’s enduring interest in geophysics and other aspects of the earth sciences is documented by his many publications on the subject. See the bibliography of Jordan’s articles and books in Beiglböck (2007).
- 98.
Jordan (1971), p. 2.
- 99.
Jordan (1959a), p. 113.
- 100.
- 101.
Fierz (1956), Goenner (2012). For a lucid summary of Jordan’s cosmological theory as developed in the late 1950s, see Heckmann and Schücking (1959). Other aspects of Jordan’s theory were dealt with in Brill (1962) and O’Hanlon and Tam (1970).
- 102.
Just (1955). On Just’s early work on Jordan’s theory, see Goenner (2012). Just later moved to the United States to become professor of physics at the University of Arizona, Tuczon.
- 103.
- 104.
- 105.
- 106.
Jordan (1969b), p. 253.
- 107.
Brans and Dicke (1961).
- 108.
Kaiser (1998).
- 109.
Brans (1961). See also Brans (1999, 2010) for personal and historical comments on the paper and on scalar–tensor theories in general. Kaiser (1998, 2007) compares the Brans–Dicke theory to the theory of the Higgs field proposed a few years later. Both theories related to the origin of mass, but they belonged to two widely different research traditions.
- 110.
Dicke (1959a).
- 111.
Jordan (1955), p. 138.
- 112.
E.g. Dicke (1964a). Mach’s principle has given rise to a very extensive literature, both philosophical and scientific. For a contemporaneous and critical discussion of its use in and relevance for cosmology and theories of gravitation, see for example Reinhardt (1973).
- 113.
Dicke (1959c), p. 621.
- 114.
Brans and Dicke (1961), Dicke (1962a).
- 115.
Dicke (1962a), p. 657.
- 116.
- 117.
Dicke (1961b), p. 100.
- 118.
On Dicke’s life and work, see Peebles (2008). Interviews with Dicke include Lightman and Brawer (1990), pp. 201–213, and three interviews conducted by the American Institute of Physics between 1975 and 1988. The interviews can be found online as http://www.aip.org/history/ohilist/transcripts.html. Dicke reprinted most of his early papers on relativity, cosmology and geophysics in a book-length chapter on “Experimental Relativity” in DeWitt and DeWitt (1964), pp. 165–316. For a review of Dicke’s work in geophysics, see Kragh (2015c).
- 119.
See Kaiser (1998) for aspects of the renaissance.
- 120.
Interview of 18 June 1985. See http://www.aip.org/history/ohilist/4572.html
- 121.
For the background of the Chapel Hill conference 18–23 January 1957, see DeWitt and Rickles (2011), which includes the reports and discussions of the conference. There were interesting links between the Chapel Hill conference and the Gravity Research Foundation (GRF) to be mentioned in Sect. 3.1. Bryce DeWitt won the first prize in the 1953 competition and was instrumental in lifting the scientific respectability of the GRF.
- 122.
Bergmann (1957). On the other hand, another of Einstein’s former German-American collaborators, Valentine Bargmann at Princeton University, covered in the same volume of Reviews of Modern Physics Jordan’s theory in a review article on the theory of relativity. Bargmann evidently found the possibility that G might vary in space and time to be interesting and worthwhile to test experimentally. See Bargmann (1957).
- 123.
Mercier and Kervaire (1956). Yet another important event in the renaissance of general relativity (including cosmology) was the 1958 Solvay Congress on “Astrophysics, Gravitation, and the Structure of the Universe,” which included addresses by Bondi, Hoyle, Wheeler, Lemaître, and Klein. Two years later the International Committee on General Relativity and Gravitation was established.
- 124.
DeWitt (2009), p. 414. According to DeWitt, Wheeler succeeded in persuading Goudsmit not to keep general relativity out of Physical Review.
- 125.
Dicke (1961c), p. 797.
- 126.
Dicke (2011), p. 58. The possibility of parity non-conservation in weak interactions had been inferred on theoretical grounds by Tsung Dao Lee and Chen Ning Yang in 1956 and was verified experimentally in early 1957. The discovery was announced at a meeting of the American Physical Society in January 1957, just in time for the physicists at the Chapel Hill conference to know about it.
- 127.
Dicke (2011), p. 53.
- 128.
Issue no. 3 of the 1957 volume of Reviews of Modern Physics contained papers prepared in connection with the Chapel Hill conference. Most of the papers, including Dicke (1957b), had not been presented at the conference but may have been informally discussed. The other paper by Dicke (1957a) followed his presentation at Chapel Hill. The issue of Reviews of Modern Physics also included Hugh Everett’s doctoral dissertation on the “relative state” formulation of quantum mechanics which in Bryce DeWitt’s later formulation became known as the many-worlds interpretation. Although Everett did not attend the Chapel Hill conference, his ideas were mentioned in the discussions.
- 129.
Dicke (1957b). On this topic, see also Sect. 4.1, footnote 1.
- 130.
Dicke (1959a), p. 29.
- 131.
Dicke (1959b). See also Peebles and Dicke (1962b). Solomon’s suggestion of 1938 resulted in a decay constant varying as t −n with n = 2/3 (see Sect. 2.2).
- 132.
- 133.
- 134.
- 135.
Bondi (1952), pp. 59–62, 159–164.
- 136.
Carter (1989), p. 190. Dyson (1972) mentioned Carter’s “principle of cognizability” in relation to Dirac’s G(t) hypothesis. The anthropic principle was introduced in Carter (1973), where Carter stated it as the opposite of the Dirac–Jordan varying-G hypothesis.
- 137.
Dicke (1962a). See Sect. 3.6 for a version of Dicke’s temperature-time graph.
- 138.
Dicke (1957a), p. 358.
- 139.
- 140.
Wigley (1981).
- 141.
Dicke (1964b), p. 160.
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Kragh, H. (2016). Varying Gravity. In: Varying Gravity. Science Networks. Historical Studies, vol 54. Birkhäuser, Cham. https://doi.org/10.1007/978-3-319-24379-5_2
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