BurchfieldJoe D., Lord Kelvin and the age of the Earth (London, 1975).
2.
HolmesArthur, The age of the Earth (New York, 1913), 120. On Holmes and his important work in geology and geophysics, see LewisCherry L. E., The dating game: One man's search for the age of the Earth (Cambridge, 2000), and idem, âArthur Holmes' vision of a geological timescaleâ, in LewisC. L. E.KnellS. J. (eds), The age of the Earth: From 4004 BC to AD 2002 (London, 2001), 121â38.
3.
The key argument is mentioned in KraghH., Matter and spirit in the universe: Scientific and religious preludes to modern cosmology (London, 2004), 192.
4.
TaitPeter G., [address by president of the mathematics and physics section], Report, British Association for the Advancement of Science, 1871, 1â8, p. 6.
5.
The literature on the entropic creation argument is limited. See LandsbergPeter T., âFrom entropy to God?â, in MartinĂ sKatalinRopolyiLĂĄszlĂłSzegediPeter (eds), Thermodynamics: History and philosophy (Singapore, 1991), 379â403; Kragh, Matter and spirit in the universe (ref. 3); and Elizabeth R. Neswald, Thermodynamik als kultureller Kampfplatz: Faszinationsgeschichte der Entropie 1850â1915 (Berlin, 2006).
6.
See SchnippenkötterJosef, Das Entropiegesetz: Seine physikalische und seine philosophische und apologetische Bedeutung (Essen, 1920) for a careful survey of the philosophical and theological aspects of the law of entropy increase. For a more recent but less detailed survey, see SeegerRaymond J., âOn humanistic aspects of entropyâ, Physis, ix (1969), 1969â34. See also KraghH., âFrom entropy to a divinely created universe: A forgotten theme in the history of science and theologyâ, in KraghH. (ed.), Theology and science: Issues for future dialogue (Aarhus, 2006), 61â88.
7.
YoungCharles A., A text-book of general astronomy (Boston, 1893), 524â5. The reference is to 2 Peter 3:13.
KolhörsterWerner, Die durchdringende Strahlung in der AtmosphĂ€re (Hamburg, 1924). On the origin of research in cosmic rays, see XuQiaozhenBrownLaurie, âThe early history of cosmic ray researchâ, American journal of physics, lv (1987), 1987â33.
10.
FarringtonOliver, âThe constitution of meteoritesâ, Journal of geology, ix (1901), 393â408, 522â32.
11.
StoneS. Bradford, âThe origin of the chemical elementsâ, Journal of physical chemistry, xxxiv (1930), 821â41, p. 827.
12.
This insight was reached principally by PayneCeciliaRussellHenry NorrisUnsöldAlbrechtStrömgrenBengt, and EddingtonArthur. See HufbauerKarl, Exploring the Sun: Solar science since Galileo (Baltimore, 1991), 101â6. See also DeVorkinDavid H.KenatRalph, âQuantum physics and the stars II: The abundances of the elements in the atmospheres of the Sun and the starsâ, Journal for the history of astronomy, xiv (1983), 1983â222, and DeVorkinD. H., Henry Norris Russell: Dean of American astronomers (Princeton, 2000), 199â218.
13.
CampbellNorman R., âThe radiation from ordinary materialsâ, Philosophical magazine, ix (1905â6), 531â44; xi (1906), 206â24.
14.
Rutherford, Radioactive transformations (ref. 8), 217. Rutherford's âgeneral principleâ crumbled as radioactivity was further investigated, and it was contradicted by the discovery of superconductivity a few years later. Mercury, tin and lead turned out to be superconductors, whereas platinum, gold and most other metals were ordinary conductors. Physicists and chemists were puzzled as to why only some elements had superconducting properties, and did not form a recognizable pattern in the periodic system. For details, see DahlPer F., Superconductivity: Its historical roots and development from mercury to the ceramic oxides (New York, 1992).
15.
CampbellN. R., Modern electrical theory (Cambridge, 1907), 213.
16.
CrookesWilliam, Modern views of matter: The realisation of a dream (Berlin, 1903), 16. Crookes speculated that the world had originally consisted of a formless collection of electrons (or other elementary particles) out of which atoms had been formed; because of their inbuilt instability the atoms would eventually return to the original state (and perhaps this process of a cosmic cycle would go on endlessly).
17.
See ElsterJuliusGeitelHans, âEntdeckungsgeschichte und Grundtatsachen der RadioaktivitĂ€tâ, in WarburgEmil (ed.), Physik (Leipzig, 1915), 478â94, pp. 488â91. Elster and Geitel did not believe in the hypothesis, but would not rule it out either.
18.
See HufbauerK., âAstronomers take up the stellar-energy problemâ, Historical studies in the physical sciences, xi (1981), 277â303, pp. 280â2.
19.
WilsonW. E., âRadium and solar energyâ, Nature, lxviii (1903), 222; DarwinGeorge H., âRadioactivity and the age of the Sunâ, Nature, lxviii (1903), 496; HardyW. B., âRadium and the cosmical time scaleâ, Nature, lxviii (1903), 548; StruttRobert J., âRadium and the Sun's heatâ, Nature, lxviii (1903), 572; and JolyJohn, âRadium and the Sun's heatâ, Nature, lxviii (1903), 572.
20.
SoddyFrederick, âRadioactivityâ, Annual reports on the progress of chemistry, i (1905), 244â80, p. 277. Reprinted in SoddyF., Radioactivity and atomic theory, ed. by TrennThaddeus J. (London, 1975), 54â90.
21.
DarwinG. H., [presidential address], Report, British Association for the Advancement of Science, 1905, 3â32, p. 29. See also RutherfordE., âRadium â The cause of the Earth's heatâ, Harper's magazine, February 1905, 390â6, reprinted in RutherfordE., The collected papers of Lord Rutherford of Nelson, ed. by ChadwickJames (3 vols, London, 1962), i, 776â85: âThere is no direct evidence that radioactive matter exists in the sun, but, from the similarity of the chemical constitution of the sun and earth, its presence is to be expectedâ (p. 784).
22.
On the early history of helium, see MeadowsArthur J., Science and controversy: A biography of Sir Norman Lockyer (London, 1972), and WeeksMary E., Discovery of the elements (Easton, PA, 1968), 757â64. Evidence for helium as a disintegration product of radioactive change was first found by Ramsay and Soddy in 1903, but it took five more years before the connection was definitely confirmed. RamsayWilliamSoddyFrederick, âGases occluded by radium bromideâ, Nature, lxviii (1903), 246, and TrennThaddeus J., The self-splitting atom: The history of the RutherfordâSoddy collaboration (London, 1977), 125.
23.
Holmes, Age of the Earth (ref. 2), 116.
24.
GiebelerH., âSpektroskopischer Beobachtungen der Nova Geminorum 2 am Bonner Refraktorâ, Astronomische Nachrichtungen, cxci, no. 4582 (1912), cols 393â402. The eminent spectroscopist Heinrich Kayser suggested a theory of the origin of novae based upon radioactivity: KayserH., âEin Versuch zur ErklĂ€rung der neuen Sterne durch radioaktive Prozesseâ, Astronomische Nachrichtungen, cxci, no. 4583 (1912), cols 421â6.
25.
JolyJ., âAn estimate of the geological age of the Earthâ, Scientific transactions of the Royal Dublin Society, ix (1899), 283â8.
26.
JolyJ., âThe age of the Earthâ, Philosophical magazine, xxii (1911), 357â80. He first made the suggestion in JolyJ., Radioactivity and geology (London, 1909). On Joly, a major player in the debate over the age of the Earth, see JacksonPatrick N. Wyse, âJohn Joly (1857â1933) and his determinations of the age of the Earthâ, in LewisKnell (eds), The age of the Earth (ref. 2), 107â19.
27.
Holmes, Age of the Earth (ref. 2), 168â9. See also the discussion on radioactivity and geology in Report, British Association for the Advancement of Science, 1915, 432â5. Whether or not the hypothesis of varying decay rates is âunphilosophicâ, it was repeated by several physicists later in the century. For example, Pascual Jordan advocated the hypothesis in 1946, in part motivated by a wish to reconcile the age of the Earth and the age of the universe, cf. Kragh, Matter and spirit in the universe (ref. 3), 181. Since then, dozens of hypotheses of varying decay rates have appeared in the physics literature.
28.
Rutherford, Radioactive transformations (ref. 8), 194, and similarly in Rutherford, Radioactive substances and their radiations (ref. 8), 623. Also Becker, âRelations of radioactivity to cosmogony and geologyâ (ref. 8), found it reasonable to assume that the decay process could be reversed (p. 125).
TraversMorris W., A life of Sir William Ramsay (London, 1956), 252. See also HammerWilliam J., Radium and other radioactive substances (New York, 1903), 18. On Kelvin's conception of radioactivity, see Kragh, âThe origin of radioactivityâ (ref. 29).
33.
ChwolsonOreste D., Hegel, Haeckel, Kossuth und das zwölfte Gebot (Braunschweig, 1908), 76.
34.
Rutherford, âRadium â The cause of the Earth's heatâ (ref. 21), 396.
35.
HaasA. E., Der erste Quantenansatz fĂŒr das Atom (Stuttgart, 1966), with a biographical introduction by Armin Hermann.
36.
HaasArthur E., âDie Physik und das kosmologische Problemâ, Archiv fĂŒr systematische Philosophie, xiii (1907), 511â25.
37.
HaasA. E., âIst die Welt in Raum und Zeit unendlich?â, Archiv fĂŒr systematische Philosophie, xviii (1912), 167â84, pp. 183â4.
MeyerS.SchweidlerE., âRadioaktive Strahlungen und Umwandlungenâ, in Warburg (ed.), Physik (ref. 17), 495â513, pp. 512â13. A similar exposition appeared in Becher, WeltgebĂ€ude (ref. 39), 280â1.
41.
NernstWalther, Das WeltgebĂ€ude im Lichte der neueren Forschung (Berlin, 1921), 1. Boltzmann's lecture, in which he denied the possibility of avoiding the heat death, was published in BoltzmannL., PopulĂ€re Schriften (Leipzig, 1905), 25â50 (p. 33).
42.
NernstW., âZur neueren Entwicklung der Thermodynamikâ, Verhandlungen der Gesellschaft deutscher Naturforscher und Ărtzte, i (1912), 100â16, pp. 105â6.
43.
LeBonGustave G., The evolution of matter (New York, 1907). BernyAdalbert, âĂber kosmische Entwicklungâ, Das Weltall, xiii (1913), 1913â24.
44.
SoddyF., âRadioactivityâ, Annual reports on the progress of chemistry, iii (1907), 333â65, p. 358. Reprinted in Soddy, Radioactivity and atomic theory (ref. 20), 113â45.
45.
SoddyF., The interpretation of radium (London, 1908), 241â2.
46.
Ibid., 189. On Soddy and his lifelong fascination by cyclic processes, see ScloveRichard E., âFrom alchemy to atomic war: Frederic Soddy's âtechnology assessmentâ of atomic energy, 1900â1915â, Science, technology, & human values, xiv (1989), 163â94.
47.
Holmes, Age of the Earth (ref. 2), 121. SpencerHerbert, First principles (London, 1911; first pub. 1862), 550.
48.
KöhlerOswald, Weltschöpfung und Weltuntergang (Stuttgart, 1895), 380. HaeckelErnst, Die WeltrÀtsel (Bonn, 1901; first edn 1899), 285. Others who explicitly used the metaphor of the universe's being a perpetuum mobile included Otto Caspari, Hans Vaihinger, Friedrich Engels and Friedrich Nietzsche (none of whom was a scientist).
49.
LeBon, The evolution of matter (ref. 43). SchefflerH., Das Wesen der Ursubstanz, die Weltschöpfung und Entstehung des Lebens enthĂŒllt durch die RadioaktivitĂ€t (Leipzig, 1906). See also TunzelmannGeorg W., A treatise on electrical theory and the problem of the universe (London 1910).
50.
Hufbauer, âAstronomers take up the stellar-energy problemâ (ref. 18).
51.
EddingtonArthur S., âThe borderland of astronomy and geologyâ, Nature, cxi (1923), 18â21, p. 19.
52.
See Kragh, Matter and spirit in the universe (ref. 3), 105, and StanleyMatthew, Practical mystic: Religion, science, and A. S. Eddington (Chicago, 2007).
53.
NernstW., âPhysico-chemical considerations in astrophysicsâ, Journal of the Franklin Institute, ccvi (1928), 135â42, p. 137. On Nernst's cosmology and its relationship to the cosmological views of MacMillanW.MillikanR., see KraghH., âCosmology between the wars: The NernstâMacMillan alternativeâ, Journal for the history of astronomy, xxvi (1995), 1995â115. For a contemporary view, see GĂŒntherPaul, âDie kosmologischen Betrachtungen von Nernstâ, Zeitschrift fĂŒr angewandte Chemie, xxxvii (1924), 1924â7. See also Kolhörster, Die durchdringende Strahlung (ref. 9), 66â67, who expressed sympathy for Nernst's ideas.
54.
Nernst, âPhysico-chemical considerations in astrophysicsâ (ref. 53), 141.
RutherfordE., âThe electrical structure of matterâ, Report, British Association for the Advancement of Science, 1923, 1â24, p. 20. This paper is not reproduced in Rutherford, Collected papers (ref. 21).
57.
StruttR. J., âSome problems of cosmical physicsâ, Report, British Association for the Advancement of Science, 1929, 49.
58.
LewisGilbert N., âThe chemistry of the stars and the evolution of radioactive substancesâ, Publications of the Astronomical Society of the Pacific, xxxiv (1922), 310â19, pp. 318â19.
59.
LewisG. N., âThe symmetry of time in physicsâ, Science, lxxi (1930), 569â77.
60.
JeansJ., âThe evolution of starsâ, Nature, cxvii (1926), 18â21, p. 21. On Jeans's conception of stellar energy and cosmic rays, see De MariaMichelangeloRussoArturo, âCosmic rays and cosmological speculations in the 1920s: The debate between Jeans and Millikanâ, in BertottiBruno (eds), Modern cosmology in retrospect (Cambridge, 1990), 401â9.
61.
JeansJ., âThe physics of the universeâ, Nature, cxxii (1928), 689â700, p. 699. Based on the first Herbert Willis Memorial Lecture, delivered on 30 October 1928.
62.
Ibid., 691. Jeans took the half-lives of uranium-238 and thorium-232 to be 5 billion years and 15 billion years, respectively. The present values are 4.5 billion years and 14 billion years.
63.
Ibid., 696.
64.
JeansJ., The universe around us (2nd edn, Cambridge, 1930), 336, preface dated 2 August 1930. The age of the universe obtained on the basis of relativistic cosmology (the Hubble time) was about 2 Ă 109 years. Jeans based his figure on his theory of the condensation of nebulae to form stars, from which followed the so-called long time-scale of about 1013 years. See BrushStephen G., âIs the Earth too old? The impact of geochronology on cosmology, 1929â1952â, in LewisKnell (eds), The age of the Earth (ref. 2), 157â75.
65.
JeansJ., The mysterious universe (Cambridge, 1930), 182. The book was based on the Rede Lecture delivered in November 1930.
66.
LemaĂźtreGeorges, âThe beginning of the world from the point of view of quantum theoryâ, Nature, cxxvii (1931), 706.
67.
LemaĂźtreG., âThe cosmological constantâ, in SchilppPaul A. (ed.), Albert Einstein: Philosopher-scientist (New York, 1949), 437â56, p. 452. A detailed examination of LemaĂźtre's motives for proposing his primeval-atom model of the universe is presented in H. Kragh and Dominique Lambert, âThe context of discovery: LemaĂźtre and the origin of the primeval-atom universeâ, Annals of science (forthcoming, 2007).
68.
LemaĂźtreG., âL'expansion de l'espaceâ, Revues des questions scientifiques, xvii (1931), 391â410. Reprinted in LemaĂźtreG., L'hypothĂšse de l'atome primitif: Essai de cosmogonie (NeuchĂątel, 1946), 67â92.
69.
LemaĂźtreG., [untitled], Nature, cxxviii (1931), 704â6, p. 705.
70.
Ibid. For LemaĂźtre's inspiration from Jeans, see KraghLambert, âThe context of discoveryâ (ref. 67).