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The abundances of light elements based on the big bang nucleosynthesis model are calculated using the Tsallis non-extensive statistics. The impact of the variation of the non-extensive parameter $q$ from the unity value is compared to…

Nuclear Theory · Physics 2015-06-05 C. A. Bertulani , J. Fuqua , M. S. Hussein

The Big Bang nucleosynthesis (BBN) in the presence of charged massive particles (CHAMPs) is studied in detail. All currently known effects due to the existence of bound states between CHAMPs and nuclei, including possible late-time…

High Energy Physics - Phenomenology · Physics 2009-06-19 Karsten Jedamzik

Uncertainties in nucleosynthesis models originating from uncertainties in astrophysical reaction rates were estimated in a Monte Carlo variation procedure. Thousands of rates were simultaneously varied within individual,…

Solar and Stellar Astrophysics · Physics 2018-06-05 T. Rauscher , N. Nishimura , G. Cescutti , R. Hirschi , A. St. J. Murphy

The current state of affairs in big-bang nucleosynthesis is reviewed and controversies are discussed. The author concludes that the glass is half full.

Astrophysics · Physics 2007-05-23 Michael S. Turner

We determine the influence of a variation of the fundamental ``constants'' on the predicted helium abundance in Big Bang Nucleosynthesis. The analytic estimate is performed in two parts: the first step determines the dependence of the…

Astrophysics · Physics 2008-11-26 Christian M. Mueller , Gregor Schaefer , Christof Wetterich

Standard Big Bang Nucleosynthesis at the baryon density determined by the microwave anisotropy spectrum predicts an excess of \li7 compared to observations by a factor of 4-5. In contrast, BBN predictions for D/H are somewhat below (but…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-04 Keith A. Olive , Patrick Petitjean , Elisabeth Vangioni , Joseph Silk

The current of status of big bang nucleosynthesis is reviewed and the concordance between theory and observation is examined in detail. It is argued that when using the observational data on he4 and li7, the two isotopes whose abundances…

Astrophysics · Physics 2008-02-03 Keith A. Olive

The successful prediction of light element abundances from Big Bang Nucleosynthesis has been a pillar of the standard model of Cosmology. Because many of the relevant reaction rates are sensitive to the values of fundamental constants, such…

High Energy Physics - Phenomenology · Physics 2009-11-11 Baojiu Li , Ming-Chung Chu

Nucleosynthesis in Type I X-ray bursts may involve up to several thousand nuclear processes. The majority of these processes have only been determined theoretically due to the lack of sufficient experimental information. Accurate reaction…

Astrophysics · Physics 2009-11-13 A. Parikh , J. Jose , C. Iliadis , F. Moreno , T. Rauscher

A detailed analysis of primordial nucleosynthesis predictions for light element abundances is performed. Contents: 1. The standard cosmology: an overview. 2. Primordial nucleosynthesis. 3. The Born rates for n<->p reactions. 4. Finite…

Astrophysics · Physics 2007-05-23 S. Esposito

A cosmological model with a time-varying mass of electrons seems a promising solution for the so-called Hubble tension. We examine the big bang nucleosynthesis (BBN) constraints on the time-varying electron mass model, because a larger…

Cosmology and Nongalactic Astrophysics · Physics 2023-05-01 Osamu Seto , Yo Toda

The 3He({\alpha},{\gamma})7Be reaction affects not only the production of 7Li in Big Bang nucleosynthesis, but also the fluxes of 7Be and 8B neutrinos from the Sun. This double role is exploited here to constrain the former by the latter. A…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-22 Marcell P. Takács , Daniel Bemmerer , Tamás Szücs , Kai Zuber

A key pillar of modern cosmology, Big Bang Nucleosynthesis (BBN) offers a probe of the particle content and expansion rate of the Universe a mere few minutes after the beginning. When compared with the BBN predictions, the observationally…

Astrophysics · Physics 2007-05-23 Gary Steigman

Following the completion of the second neutron beam line and the related experimental area (EAR2) at the n_TOF spallation neutron source at CERN, several experiments were planned and performed. The high instantaneous neutron flux available…

Instrumentation and Detectors · Physics 2018-03-14 M. Barbagallo , J. Andrzejewski , M. Mastromarco , J. Perkowski , L. A. Damone , A. Gawlik , L. Cosentino , P. Finocchiaro , E. A. Maugeri , A. Mazzone , R. Dressler , S. Heinitz , N. Kivel , D. Schumann , N. Colonna , O. Aberle , S. Amaducci , L. Audouin , M. Bacak , J. Balibrea , F. Bečvář , G. Bellia , E. Berthoumieux , J. Billowes , D. Bosnar , A. Brown , M. Caamaño , F. Calviño , M. Calviani , D. Cano-Ott , R. Cardella , A. Casanovas , F. Cerutti , Y. H. Chen , E. Chiaveri , G. Cortés , M. A. Cortés-Giraldo , S. Cristallo , M. Diakaki , M. Dietz , C. Domingo-Pardo , E. Dupont , I. Durán , B. Fernández-Domínguez , A. Ferrari , P. Ferreira , V. Furman , K. Göbel , A. R. García , S. Gilardoni , T. Glodariu , I. F. Gonçalves , E. González-Romero , E. Griesmayer , C. Guerrero , F. Gunsing , H. Harada , J. Heyse , D. G. Jenkins , E. Jericha , K. Johnston , F. Käppeler , Y. Kadi , A. Kalamara , P. Kavrigin , A. Kimura , M. Kokkoris , M. Krtička , D. Kurtulgil , C. Lederer , H. Leeb , J. Lerendegui-Marco , S. Lo Meo , S. J. Lonsdale , D. Macina , A. Manna , J. Marganiec , T. Martínez , J. G. Martins-Correia , A. Masi , C. Massimi , P. Mastinu , E. Mendoza , A. Mengoni , P. M. Milazzo , F. Mingrone , A. Musumarra , A. Negret , R. Nolte , A. Oprea , A. D. Pappalardo , N. Patronis , A. Pavlik , M. Piscopo , I. Porras , J. Praena , J. M. Quesada , D. Radeck , T. Rauscher , R. Reifarth , M. S. Robles , C. Rubbia , J. A. Ryan , M. Sabaté-Gilarte , A. Saxena , J. Schell , P. Schillebeeckx , P. Sedyshev , A. G. Smith , N. V. Sosnin , A. Stamatopoulos , G. Tagliente , J. L. Tain , A. Tarifeño-Saldivia , L. Tassan-Got , S. Valenta , G. Vannini , V. Variale , P. Vaz , A. Ventura , V. Vlachoudis , R. Vlastou , A. Wallner , S. Warren , C. Weiss , P. J. Woods , T. Wright , P. Žugec

It has been suggested that a $\nu$p process can occur when hot, dense, and proton-rich matter is expanding within a strong flux of anti-neutrinos. In such an environment, proton-rich nuclides can be produced in sequences of proton captures…

Solar and Stellar Astrophysics · Physics 2019-09-02 N. Nishimura , T. Rauscher , R. Hirschi , G. Cescutti , A. St. J. Murphy , C. Fröhlich

Big Bang Nucleosynthesis can provide, via constraints on the expansion rate at that time, limits on possible variations in Newton's Constant, $G$. The original analyses were performed before an independent measurement of the…

Astrophysics · Physics 2009-11-10 Craig J. Copi , Adam N. Davis , Lawrence M. Krauss

We present a new astrophysical site of the big bang nucleosynthesis (BBN) that are very peculiar compared with the standard BBN. Some models of the baryogenesis suggest that very high baryon density regions were formed in the early…

Astrophysics · Physics 2009-11-13 S. Matsuura , S. Fujimoto , S. Nishimura , M. Hashimoto , K. Sato

We include correlations between elemental abundances in a Monte Carlo statistical analysis of BBN predictions, which, along with updated reaction rates and an improved BBN code, lead to tightened constraints on $\Omega_{B}$ and $N_{\nu}$.…

Astrophysics · Physics 2009-10-22 Peter J. Kernan , Lawrence M. Krauss

The study of d+d reactions is of major interest since their reaction rates affect the predicted abundances of D, 3He, and 7Li. In particular, recent measurements of primordial D/H ratios call for reduced uncertainties in the theoretical…

Instrumentation and Methods for Astrophysics · Physics 2017-11-15 Á. Gómez Iñesta , C. Iliadis , A. Coc

The role of neutrinos in big bang nucleosynthesis is discussed. The bounds on the number of neutrino families, neutrino degeneracy, parameters of neutrino oscillations are presented. A model of chemically inhomogeneous, while energetically…

High Energy Physics - Phenomenology · Physics 2010-11-11 A. D. Dolgov
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