Big Bang Photosynthesis and Pregalactic Nucleon Synthesis of Light Elements

1985
24 pages
Published in:
  • Astrophys.J.Lett. 293 (1985) L53-L57
Report number:
  • FERMILAB-PUB-84-121-A

Citations per year

19861995200420132022012345
Abstract: (ADS)
Two nonstandard scenarios for pregalactic synthesis of the light elements (2H, 3He, 4He, and 7Li) are developed. Big bang photosynthesis occurs if energetic photons, produced by the decay of massive neutrinos or gravitinos, partially photodisintegrate 4He (formed in the standard hot big bang) to produce 2H and 3He. In this case, primordial nucleosynthesis no longer constrains the baryon density of the universe, or the number of neutrino species. Alternatively, one may dispense partially or completely with the hot big bang and produce the light elements by bombardment of primordial gas, provided that 4He is synthesized by a later generation of massive stars.
  • COSMOLOGICAL MODEL
  • FUSION
  • LIGHT NUCLEUS: PRODUCTION
  • PRODUCTION: LIGHT NUCLEUS
  • HYDROGEN
  • HELIUM: NUCLIDE
  • LITHIUM
  • HELIUM: PHOTOFISSION
  • BARYON: DENSITY
  • NEUTRINO: MASS
  • 19
    • preprint (Space Science
      • F. Aharonian
        ,
      • R.A. Sunyaev
    • Research Institute)
      • in Primordial Helium, P. Shaver, D. Kunth, and K. Kjar (eds.) (European Southern Observatory: Garching), p. 71
        • J. Audouze
          ,
        • J. Silk
      • in Proc. First ESO-CERN Symposium, Large-Scale
        • J. Audouze
      • Structure of the Universe, Cosmology, and Fundamental Physics, eds
        • (CERN: Geneva), p. 293
          • C. Setti
            ,
          • L. Van Hove
            • J.R. Bond
              ,
            • B.J. Carr
              ,
            • W.D. Arnett
              • Nature 304 (1983) 514
          • in Proc. HEP-83, International Europhysics
            • S. Boris
          • Conference on High Energy Physics and C. Cost&n
            • J. Guy
            • (Rutherford Appleton Laboratory: Chilton), p. 386
                • Delbourgo-Salvador
                  ,
                • C. P.. Gry
                  ,
                • G. Malinie
                  ,
                • J. Audouze
              • Astr. Ap. in press
                • Ap. J., 2. 327
                  • D.A. Dicus
                    ,
                  • E.W. Kolb
                    ,
                  • V.L. Teplitz
                • v., CERN preprint TH 3839
                  • J. Ellis
                    ,
                  • J. Kim
                    ,
                  • D. Nanopoulos
                • AP. J., E. 595
                  • R. Epstein
                • 20
                  • Proc. First ESO-CERN Symposium, lot. cit., P. 35
                    • P. Fayet
                    • D. Gautier
                      ,
                    • R. Owen
                      • Nature 302 (1983) 215
                    • P. Hut
                      ,
                    • S.D.M. White
                      • Nature 2 (1984) 637
                    • D. Lindley
                      • Mon.Not.Roy.Astron.Soc. 2 (1979) 15
                  • Ap. J., (submitted)
                    • D. Lindley
                    • V. Lyubimov
                      ,
                    • E. Novikov
                      ,
                    • V. Notik
                      ,
                    • E. Tretyakov
                      ,
                    • U. Kozik
                      • Phys.Lett. 9 266