Heller M, Woodin W.H. (eds.) Infinity. New research frontiers (CUP, 2011)(ISBN 1107003873)(O)(327s)_MAml_

Heller M, Woodin W.H. (eds.) Infinity. New research frontiers (CUP, 2011)(ISBN 1107003873)(O)(327s)_MAml_ Heller M, Woodin W.H. (eds.) Infinity. New research frontiers (CUP, 2011)(ISBN 1107003873)(O)(327s)_MAml_

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eferences 215Bersanelli, M. 2005. An echo of ancient questions from contemporary cosmology. In 100 Perspectiveson Science and Religion, Charles L. Harper, Jr. (ed.), pp. 121–26. Philadelphia and London:Templeton Foundation Press. Publication in honor of Sir John Templeton.Bersanelli, M., and Gargantini, M. 2009. From Galileo to Gelmann: The Wonder that Inspiredthe Greatest Scientists of All Time In Their Own Words. Philadelphia and London: TempletonFoundation Press.Bersanelli, M., Maino, D., and Mennella, A. 2002. Anisotropies of the cosmic microwave background.La Rivista del Nuovo Cimento 25: 1.Beveridge, W. I. B. 1950. The Art of Scientific Investigation. London: William Heinemann.Bousso, R. 2006. Holographic probabilities in eternal inflation. Physical Review Letters 97: 191302.Boyle, L. A., Steinhardt, P. J., and Turok, N. 2006. Inflationary predictions for scalar and tensorfluctuations reconsidered. Physical Review Letters 96: 111301.Brose, M. 1983. Leopardi’s “L’infinito” and the language of the romantic sublime. Poetics Today 4:1,47–71.Chaboyer, B., and Krauss, L. M. 2002. Theoretical uncertainties in the subgiant mass-age relationand the absolute age of ω Centauri. Astrophysical Journal 567: L45.Chandrasekhar, S. 1990. Truth and Beauty. Aesthetics and Motivation in Science. Chicago: Universityof Chicago Press.Cole, S., et al. 2005. The 2dF Galaxy Redshift Survey: Power-spectrum analysis of the final data setand cosmological implications. Monthly Notices of the Royal Astronomical Society 362: 505.Dante Alighieri. Inferno XXXIV 139; Purgatorio XXXIII 145; Paradiso XXXIII 145. Commentedby Attilio Momigliano (1974). Firenze: Sansoni Editore.Dostoevsky, F. 1872. The Devils, p. 656. Translated by David Magarshack (1971). Middlesex:Penguin Books.Dunkley, J., et al. 2005. Measuring the geometry of the universe in presence of isocurvature modes.Physical Review Letters 95: 261303.Dyson, L., Kleban, M., and Susskind, L. 2002. Disturbing implications of a cosmological constant.Journal of High Energy Physics 0210, 011., vol. 10, n. 11.Eisenstein, D. J., et al. 2005. Detection of the baryon acoustic peak in the large-scale correlationfunction of SDSS luminous red galaxies. Astrophysical Journal 633: 560.Ellis, G. F. R. 1971. Relativistic cosmology. In General Relativity and Cosmology, Proceedings ofthe XLVII Enrico Fermi Summer School, R. K. Sachs (ed.). New York: Academic Press. Pag. 104.Ellis, G. F. R. 2006. Issues in the Philosophy of Cosmology, Handbook in Philosophy of Physics,J. Butterfield and J. Earman (eds.). Amsterdam: Elsevier.Ellis, G. F. R., Kirchner, U., and Stoeger, W. R. 2004. Multiverses and physical cosmology. MonthlyNotices of the Royal Astronomical Society 347: 921.Escher, M.C. 1952. Cubic Space Division, 27× 26.5 cm, Cordon Art, Baarn, Holland.Escher, M. C. 1955. Depth, 32× 23 cm. Cordon Art, Baarn, Holland.Freedman, W. L., et al. 2001. Final results from the Hubble Space Telescope Key Project to measurethe Hubble constant. Astrophysical Journal 553: 47.Friedrich, C. D. 1809. Monk by the Sea, 110 × 171.5 cm. Gemäldegalerie, Berlín, Germany.Friedrich, C. D. 1818. The Wanderer above a Sea of Mists, 74.8 × 94.8 cm. Hamburger Kunsthalle,Hamburg, Germany.Garnavich, P. M., et al. 1998. Constraints on cosmological models from Hubble Space Telescopeobservations of high-z supernovae. Astrophysical Journal 493: L53.Giulini, D., Joos, E., Kiefer, C., et al. 1996. Decoherence and the Appearance of a Classical Worldin Quantum Theory. Berlin: Springer.Giussani, L. 1997. The Religious Sense. Translated by J. Zucchi. Montreal: McGill-Queen’s UniversityPress.

eferences 215Bersanelli, M. 2005. An echo of ancient questions from contemporary cosmology. In 100 Perspectiveson Science and Religion, Charles L. Harper, Jr. (ed.), pp. 121–26. Philadelphia and London:Templeton Foundation Press. Publication in honor of Sir John Templeton.Bersanelli, M., and Gargantini, M. 2009. From Galileo to Gelmann: The Wonder that Inspiredthe Greatest Scientists of All Time In Their Own Words. Philadelphia and London: TempletonFoundation Press.Bersanelli, M., Maino, D., and Mennella, A. 2002. Anisotropies of the cosmic microwave background.La Rivista del Nuovo Cimento 25: 1.Beveridge, W. I. B. 1950. The Art of Scientific Investigation. London: William Heinemann.Bousso, R. 2006. Holographic probabilities in eternal inflation. Physical Review Letters 97: 191302.Boyle, L. A., Steinhardt, P. J., and Turok, N. 2006. Inflationary predictions for scalar and tensorfluctuations reconsidered. Physical Review Letters 96: 111301.Brose, M. 1983. Leopardi’s “L’infinito” and the language of the romantic sublime. Poetics Today 4:1,47–71.Chaboyer, B., and Krauss, L. M. 2002. Theoretical uncertainties in the subgiant mass-age relationand the absolute age of ω Centauri. Astrophysical Journal 567: L45.Chandrasekhar, S. 1990. Truth and Beauty. Aesthetics and Motivation in Science. Chicago: Universityof Chicago Press.Cole, S., et al. 2005. The 2dF Galaxy R<strong>eds</strong>hift Survey: Power-spectrum analysis of the final data setand cosmological implications. Monthly Notices of the Royal Astronomical Society 362: 505.Dante Alighieri. Inferno XXXIV 139; Purgatorio XXXIII 145; Paradiso XXXIII 145. Commentedby Attilio Momigliano (1974). Firenze: Sansoni Editore.Dostoevsky, F. 1872. The Devils, p. 656. Translated by David Magarshack (1971). Middlesex:Penguin Books.Dunkley, J., et al. 2005. Measuring the geometry of the universe in presence of isocurvature modes.Physical Review Letters 95: 261303.Dyson, L., Kleban, M., and Susskind, L. 2002. Disturbing implications of a cosmological constant.Journal of High Energy Physics 0210, 011., vol. 10, n. 11.Eisenstein, D. J., et al. 2005. Detection of the baryon acoustic peak in the large-scale correlationfunction of SDSS luminous red galaxies. Astrophysical Journal 633: 560.Ellis, G. F. R. 1971. Relativistic cosmology. In General Relativity and Cosmology, Proceedings ofthe XLVII Enrico Fermi Summer School, R. K. Sachs (ed.). <strong>New</strong> York: Academic Press. Pag. 104.Ellis, G. F. R. 2006. Issues in the Philosophy of Cosmology, Handbook in Philosophy of Physics,J. Butterfield and J. Earman (<strong>eds</strong>.). Amsterdam: Elsevier.Ellis, G. F. R., Kirchner, U., and Stoeger, W. R. 2004. Multiverses and physical cosmology. MonthlyNotices of the Royal Astronomical Society 347: 921.Escher, M.C. 1952. Cubic Space Division, 27× 26.5 cm, Cordon Art, Baarn, Holland.Escher, M. C. 1955. Depth, 32× 23 cm. Cordon Art, Baarn, Holland.Freedman, W. L., et al. 2001. Final results from the Hubble Space Telescope Key Project to measurethe Hubble constant. Astrophysical Journal 553: 47.Friedrich, C. D. 1809. Monk by the Sea, 110 × 171.5 cm. Gemäldegalerie, Berlín, Germany.Friedrich, C. D. 1818. The Wanderer above a Sea of Mists, 74.8 × 94.8 cm. Hamburger Kunsthalle,Hamburg, Germany.Garnavich, P. M., et al. 1998. Constraints on cosmological models from Hubble Space Telescopeobservations of high-z supernovae. Astrophysical Journal 493: L53.Giulini, D., Joos, E., Kiefer, C., et al. 1996. Decoherence and the Appearance of a Classical Worldin Quantum Theory. Berlin: Springer.Giussani, L. 1997. The Religious Sense. Translated by J. Zucchi. Montreal: McGill-Queen’s UniversityPress.

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