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Big Bang Nucleosynthesis (BBN) and the Cosmic Background Radiation (CBR) provide complementary probes of the early evolution of the Universe and of its particle content. Neutrinos play important roles in both cases, influencing the…

高能物理 - 唯象学 · 物理学 2008-11-26 Gary Steigman

We describe the main features of a new and updated version of the program PArthENoPE, which computes the abundances of light elements produced during Big Bang Nucleosynthesis. As the previous first release in 2008, the new one, PArthENoPE…

宇宙学与河外天体物理 · 物理学 2018-08-28 R. Consiglio , P. F. de Salas , G. Mangano , G. Miele , S. Pastor , O. Pisanti

The initial conditions of our Universe can be summarized on a single sheet of paper. Yet the Universe is full of complex structures today, such as stars, galaxies and groups of galaxies. In this review I describe the standard theoretical…

天体物理学 · 物理学 2008-04-16 Abraham Loeb

We discuss the effects of a possible time variation of the Newton constant $G_{\rm N}$ on light elements production in Big Bang Nucleosyntesis (BBN). We provide analytical estimates for the dependence of primordial abundances on the value…

天体物理学 · 物理学 2008-11-26 C. Bambi , M. Giannotti , F. L. Villante

We reinvestigate the constraints from primordial nucleosynthesis on a possible time-dependent quark mass. The limits on such quark-mass variations are particularly sensitive to the adopted observational abundance constraints. Hence, in the…

宇宙学与河外天体物理 · 物理学 2014-05-06 Myung-Ki Cheoun , Toshitaka Kajino , Motohiko Kusakabe , Grant J. Mathews

Based on a scenario of the inhomogeneous big-bang nucleosynthesis (IBBN), we investigate the detailed nucleosynthesis that includes the production of heavy elements beyond Li-7. From the observational constraints on light elements of He4…

宇宙学与河外天体物理 · 物理学 2013-07-08 Riou Nakamura , Masa-aki Hashimoto , Shin-ichiro Fujimoto , Nobuya Nishimura , Katsuhiko Sato

The cosmic microwave background and the cosmic expansion can be interpreted as evidence that the Universe underwent an extremely hot and dense phase about 14 Gyr ago. The nucleosynthesis computations tell us that the Universe emerged from…

太阳与恒星天体物理 · 物理学 2015-05-18 Piercarlo Bonifacio

The first massive stars triggered the onset of chemical evolution by releasing the first metals (elements heavier than helium) in the Universe. The nature of these stars and how the early chemical enrichment took place is still largely…

太阳与恒星天体物理 · 物理学 2020-12-09 Arthur Choplin , Raphael Hirschi

The determination of the primeval deuterium abundance has opened a precision era in big-bang nucleosynthesis (BBN), making accurate predictions more important than ever before. We present in analytic form new, more precise predictions for…

天体物理学 · 物理学 2009-10-31 Scott Burles , Kenneth M. Nollett , Michael S. Turner

A brief overview of non-standard big bang nucleosynthesis (BBN) scenarios is presented. Trends and results of the light-element nucleosynthesis in BBN scenarios with small-scale or large-scale inhomogeneity, the presence of antimatter…

天体物理学 · 物理学 2007-05-23 Karsten Jedamzik

We investigate the modifications to predictions for the abundances of light elements from standard Big-Bang nucleosynthesis when exotic late-decaying particles with lifetimes exceeding ~1 sec are prominent in the early Universe. Utilising a…

I review standard big bang nucleosynthesis and some versions of nonstandard BBN. The abundances of the primordial isotopes D, He-3, and Li-7 produced in standard BBN can be calculated as a function of the baryon density with an accuracy of…

天体物理学 · 物理学 2021-04-28 Hannu Kurki-Suonio

We investigate nucleosynthesis and element formation in the early universe in the framework of higher dimensional cosmology. For this purpose we utilize a previous solution of the present author, which may be termed as the generalized…

广义相对论与量子宇宙学 · 物理学 2015-05-14 S. Chatterjee

The effects of radiatively decaying, long-lived particles on big-bang nucleosynthesis (BBN) are discussed. If high-energy photons are emitted after BBN, they may change the abundances of the light elements through photodissociation…

高能物理 - 唯象学 · 物理学 2008-11-26 Erich Holtmann , M. Kawasaki , K. Kohri , Takeo Moroi

Big-bang nucleosynthesis is one of the cornerstones of the standard cosmology. For almost thirty years its predictions have been used to test the big-bang model to within a fraction of a second of the bang. The concordance that exists…

天体物理学 · 物理学 2009-10-22 Craig J Copi , David N. Schramm , Michael S. Turner

The exactly solvable quantum model of the homogeneous, isotropic and closed universe in the matter-energy production epoch is considered. It is assumed that the universe is originally filled with a uniform scalar field and a perfect fluid…

广义相对论与量子宇宙学 · 物理学 2011-07-19 V. E. Kuzmichev , V. V. Kuzmichev

Big Bang nucleosynthesis produces only light elements and the very first generation stars are thus formed from metal-free clouds. They start the production of heavy elements during their life, and enrich the interstellar medium through…

天体物理学 · 物理学 2008-11-26 Sylvia Ekström , Georges Meynet , André Maeder

Due to their production sites, as well as to how they are processed and destroyed in stars, the light elements are excellent tools to investigate a number of crucial issues in modern astrophysics: from stellar structure and non-standard…

星系天体物理 · 物理学 2021-03-23 Sofia Randich , Laura Magrini

We present a detailed study of inhomogeneous Big Bang nucleosynthesis where, for the first time, nuclear reactions are coupled to all significant fluctuation dissipation processes. Theses processes include neutrino heat transport, baryon…

天体物理学 · 物理学 2009-10-22 K. Jedamzik , G. M. Fuller , G. J. Mathews

Primordial nucleosynthesis is rightly hailed as one of the great successes of the standard cosmological model. Here we consider the initial forging of elements in the recently proposed Rh = ct universe, a cosmology that demands linear…

宇宙学与河外天体物理 · 物理学 2016-05-25 Geraint F. Lewis , Luke A. Barnes , Rajesh Kaushik
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