Peratt, Anthony (February 1992). "Plasma Cosmology"(PDF). Sky & Telescope. 83 (2): 136–141. Retrieved 26 May 2012. recount: It was described as this in the February 1992 issue of Sky & Telescope ("Plasma Cosmology"), and by Anthony Peratt in the 1980s, who describes it as a "nonstandard picture". The ΛCDM model big bang picture is typically described as the "concordance model", "standard model" or "standard paradigm" of cosmology here[permanent dead link], and here.
Colafrancesco, S.; Giordano, F. (2006). "The impact of magnetic field on the cluster M – T relation". Astronomy and Astrophysics. 454 (3): L131–134. arXiv:astro-ph/0701852. Bibcode:2006A&A...454L.131C. doi:10.1051/0004-6361:20065404. S2CID1477289. recount: "Numerical simulations have shown that the wide-scale magnetic fields in massive clusters produce variations of the cluster mass at the level of ~ 5 − 10% of their unmagnetized value ... Such variations are not expected to produce strong variations in the relative [mass-temperature] relation for massive clusters."
Spergel, D. N.; et al. (2003). "(WMAP collaboration), "First year Wilkinson Microwave Anisotropy Probe (WMAP) observations: Determination of cosmological parameters". Astrophysical Journal Supplement Series. 148 (1): 175–194. arXiv:astro-ph/0302209. Bibcode:2003ApJS..148..175S. doi:10.1086/377226. S2CID10794058.
Bostick, W. H. (1986). "What laboratory-produced plasma structures can contribute to the understanding of cosmic structures both large and small". IEEE Transactions on Plasma Science. PS-14 (6): 703–717. Bibcode:1986ITPS...14..703B. doi:10.1109/TPS.1986.4316621. S2CID25575722.
Colafrancesco, S.; Giordano, F. (2006). "The impact of magnetic field on the cluster M – T relation". Astronomy and Astrophysics. 454 (3): L131–134. arXiv:astro-ph/0701852. Bibcode:2006A&A...454L.131C. doi:10.1051/0004-6361:20065404. S2CID1477289. recount: "Numerical simulations have shown that the wide-scale magnetic fields in massive clusters produce variations of the cluster mass at the level of ~ 5 − 10% of their unmagnetized value ... Such variations are not expected to produce strong variations in the relative [mass-temperature] relation for massive clusters."
Audouze, J.; Lindley, D.; Silk, J. (1985). "Big Bang Photosynthesis and Pregalactic Nucleosynthesis of Light Elements". Astrophysical Journal. 293: L53–L57. Bibcode:1985ApJ...293L..53A. doi:10.1086/184490.
Epstein; et al. (1976). "The origin of deuterium". Nature. 263 (5574): 198–202. Bibcode:1976Natur.263..198E. doi:10.1038/263198a0. S2CID4213710. point out that if proton fluxes with energies greater than 500 MeV were intense enough to produce the observed levels of deuterium, they would also produce about 1000 times more gamma rays than are observed.
Bostick, W. H. (1986). "What laboratory-produced plasma structures can contribute to the understanding of cosmic structures both large and small". IEEE Transactions on Plasma Science. PS-14 (6): 703–717. Bibcode:1986ITPS...14..703B. doi:10.1109/TPS.1986.4316621. S2CID25575722.
Colafrancesco, S.; Giordano, F. (2006). "The impact of magnetic field on the cluster M – T relation". Astronomy and Astrophysics. 454 (3): L131–134. arXiv:astro-ph/0701852. Bibcode:2006A&A...454L.131C. doi:10.1051/0004-6361:20065404. S2CID1477289. recount: "Numerical simulations have shown that the wide-scale magnetic fields in massive clusters produce variations of the cluster mass at the level of ~ 5 − 10% of their unmagnetized value ... Such variations are not expected to produce strong variations in the relative [mass-temperature] relation for massive clusters."
Audouze, J.; Lindley, D.; Silk, J. (1985). "Big Bang Photosynthesis and Pregalactic Nucleosynthesis of Light Elements". Astrophysical Journal. 293: L53–L57. Bibcode:1985ApJ...293L..53A. doi:10.1086/184490.
Epstein; et al. (1976). "The origin of deuterium". Nature. 263 (5574): 198–202. Bibcode:1976Natur.263..198E. doi:10.1038/263198a0. S2CID4213710. point out that if proton fluxes with energies greater than 500 MeV were intense enough to produce the observed levels of deuterium, they would also produce about 1000 times more gamma rays than are observed.
Spergel, D. N.; et al. (2003). "(WMAP collaboration), "First year Wilkinson Microwave Anisotropy Probe (WMAP) observations: Determination of cosmological parameters". Astrophysical Journal Supplement Series. 148 (1): 175–194. arXiv:astro-ph/0302209. Bibcode:2003ApJS..148..175S. doi:10.1086/377226. S2CID10794058.
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Ref. 10 in "Galactic Model of Element Formation" (Lerner, IEEE Transactions on Plasma Science Vol. 17, No. 2, April 1989 [3]Archived 2006-12-29 at the Wayback Machine) is J.Audouze and J.Silk, "Pregalactic Synthesis of Deuterium" in Proc. ESO Workshop on "Primordial Helium", 1983, pp. 71–75 [4] Lerner includes a paragraph on "Gamma Rays from D Production" in which he claims that the expected gamma ray level is consistent with the observations. He cites neither Audouze nor Epstein in this context, and does not explain why his result contradicts theirs.
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Ref. 10 in "Galactic Model of Element Formation" (Lerner, IEEE Transactions on Plasma Science Vol. 17, No. 2, April 1989 [3]Archived 2006-12-29 at the Wayback Machine) is J.Audouze and J.Silk, "Pregalactic Synthesis of Deuterium" in Proc. ESO Workshop on "Primordial Helium", 1983, pp. 71–75 [4] Lerner includes a paragraph on "Gamma Rays from D Production" in which he claims that the expected gamma ray level is consistent with the observations. He cites neither Audouze nor Epstein in this context, and does not explain why his result contradicts theirs.
Peratt, Anthony (February 1992). "Plasma Cosmology"(PDF). Sky & Telescope. 83 (2): 136–141. Retrieved 26 May 2012. recount: It was described as this in the February 1992 issue of Sky & Telescope ("Plasma Cosmology"), and by Anthony Peratt in the 1980s, who describes it as a "nonstandard picture". The ΛCDM model big bang picture is typically described as the "concordance model", "standard model" or "standard paradigm" of cosmology here[permanent dead link], and here.
Bostick, W. H. (1986). "What laboratory-produced plasma structures can contribute to the understanding of cosmic structures both large and small". IEEE Transactions on Plasma Science. PS-14 (6): 703–717. Bibcode:1986ITPS...14..703B. doi:10.1109/TPS.1986.4316621. S2CID25575722.
Colafrancesco, S.; Giordano, F. (2006). "The impact of magnetic field on the cluster M – T relation". Astronomy and Astrophysics. 454 (3): L131–134. arXiv:astro-ph/0701852. Bibcode:2006A&A...454L.131C. doi:10.1051/0004-6361:20065404. S2CID1477289. recount: "Numerical simulations have shown that the wide-scale magnetic fields in massive clusters produce variations of the cluster mass at the level of ~ 5 − 10% of their unmagnetized value ... Such variations are not expected to produce strong variations in the relative [mass-temperature] relation for massive clusters."
Epstein; et al. (1976). "The origin of deuterium". Nature. 263 (5574): 198–202. Bibcode:1976Natur.263..198E. doi:10.1038/263198a0. S2CID4213710. point out that if proton fluxes with energies greater than 500 MeV were intense enough to produce the observed levels of deuterium, they would also produce about 1000 times more gamma rays than are observed.
Peratt, Anthony (February 1992). "Plasma Cosmology"(PDF). Sky & Telescope. 83 (2): 136–141. Retrieved 26 May 2012. recount: It was described as this in the February 1992 issue of Sky & Telescope ("Plasma Cosmology"), and by Anthony Peratt in the 1980s, who describes it as a "nonstandard picture". The ΛCDM model big bang picture is typically described as the "concordance model", "standard model" or "standard paradigm" of cosmology here[permanent dead link], and here.
Ref. 10 in "Galactic Model of Element Formation" (Lerner, IEEE Transactions on Plasma Science Vol. 17, No. 2, April 1989 [3]Archived 2006-12-29 at the Wayback Machine) is J.Audouze and J.Silk, "Pregalactic Synthesis of Deuterium" in Proc. ESO Workshop on "Primordial Helium", 1983, pp. 71–75 [4] Lerner includes a paragraph on "Gamma Rays from D Production" in which he claims that the expected gamma ray level is consistent with the observations. He cites neither Audouze nor Epstein in this context, and does not explain why his result contradicts theirs.
