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Big Bang Nucleosynthesis (BBN) is studied within the framework of a two-parameter family of tensor-scalar theories of gravitation, with nonlinear scalar-matter coupling function a(phi). We run a BBN code modified by tensor-scalar gravity,…

天体物理学 · 物理学 2009-10-30 Thibault Damour , Bernard Pichon

In the framework of the standard, hot big bang cosmological model the dynamics of the early evolution of the universe is controlled by the energy density of relativistic particles, among which neutrinos play an important role. In…

天体物理学 · 物理学 2007-05-23 Gary Steigman

There are ongoing efforts in detecting Hawking radiation from primordial black holes (PBH) formed during the early universe. Here we put an upper limit on the PBH number density that could have been formed prior to the big bang…

综合物理 · 物理学 2010-06-29 C. Sivaram , Kenath Arun

Primordial nucleosynthesis is one of the three historical evidences for the big bang model, together with the expansion of the universe and the cosmic microwave background. Now that the number of neutrino families and the baryonic densities…

宇宙学与河外天体物理 · 物理学 2025-02-07 Cyril Pitrou , Alain Coc , Jean-Philippe Uzan , Elisabeth Vangioni

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 the effect on the Big Bang Nucleosynthesis (BBN) from the presence of a stochastic primordial magnetic field (PMF) whose strength is spatially inhomogeneous. We assume a uniform total energy density and a gaussian…

宇宙学与河外天体物理 · 物理学 2019-02-27 Yudong Luo , Toshitaka Kajino , Motohiko Kusakabe , Grant J. Mathews

Primordial nucleosynthesis is considered a success story of the standard big bang (SBB) cosmology. The cosmological and elementary particle physics parameters are believed to be severely constrained by the requirement of correct abundances…

天体物理学 · 物理学 2007-05-23 Daksh Lohiya , Shobhit Mahajan , A. Mukherjee , Annu Batra

We consider the effects on big bang nucleosynthesis (BBN) of the radiative decay of a long-lived massive particle. If high-energy photons are emitted after the BBN epoch ($t \sim 1 - 10^3$ sec), they may change the abundances of the light…

高能物理 - 唯象学 · 物理学 2011-05-05 M. Kawasaki , K. Kohri , Takeo Moroi

There may be non-thermal cosmic rays during big-bang nucleosynthesis (BBN) epoch (dubbed as BBNCRs). This paper investigated whether such BBNCRs can be the origin of Lithium problem or not. It can be expected that BBNCRs flux will be small…

宇宙学与河外天体物理 · 物理学 2015-05-30 Ming-ming Kang , Yang Hu , Hong-bo Hu , Shou-hua Zhu

We consider the big bang nucleosynthesis (BBN) in the Brane world scenario, where all matter fields are confined on our 3-brane and the radion of the Brane evolves cosmologically. In the Einstein frame fundamental fermion masses vary and…

天体物理学 · 物理学 2009-11-13 Baojiu Li , Ming-Chung Chu

The theoretical predictions of the primordial abundances of elements in the big-bang nucleosynthesis (BBN) are dominated by uncertainties in the input nuclear reaction rates. We investigate the effect of modifying these reaction rates on…

核理论 · 物理学 2014-06-03 Abhishek Mishra , D. N. Basu

The hot dense environment of the early universe is known to have produced large numbers of baryons, photons, and neutrinos. These extreme conditions may have also produced other long-lived species, including new light particles (such as…

宇宙学与河外天体物理 · 物理学 2019-03-13 Daniel Green , Mustafa A. Amin , Joel Meyers , Benjamin Wallisch , Kevork N. Abazajian , Muntazir Abidi , Peter Adshead , Zeeshan Ahmed , Behzad Ansarinejad , Robert Armstrong , Carlo Baccigalupi , Kevin Bandura , Darcy Barron , Nicholas Battaglia , Daniel Baumann , Keith Bechtol , Charles Bennett , Bradford Benson , Florian Beutler , Colin Bischoff , Lindsey Bleem , J. Richard Bond , Julian Borrill , Elizabeth Buckley-Geer , Cliff Burgess , John E. Carlstrom , Emanuele Castorina , Anthony Challinor , Xingang Chen , Asantha Cooray , William Coulton , Nathaniel Craig , Thomas Crawford , Francis-Yan Cyr-Racine , Guido D'Amico , Marcel Demarteau , Olivier Doré , Duan Yutong , Joanna Dunkley , Cora Dvorkin , John Ellison , Alexander van Engelen , Stephanie Escoffier , Tom Essinger-Hileman , Giulio Fabbian , Jeffrey Filippini , Raphael Flauger , Simon Foreman , George Fuller , Marcos A. G. Garcia , Juan García-Bellido , Martina Gerbino , Vera Gluscevic , Satya Gontcho A Gontcho , Krzysztof M. Górski , Daniel Grin , Evan Grohs , Jon E. Gudmundsson , Shaul Hanany , Will Handley , J. Colin Hill , Christopher M. Hirata , Renée Hložek , Gilbert Holder , Shunsaku Horiuchi , Dragan Huterer , Kenji Kadota , Marc Kamionkowski , Ryan E. Keeley , Rishi Khatri , Theodore Kisner , Jean-Paul Kneib , Lloyd Knox , Savvas M. Koushiappas , Ely D. Kovetz , Benjamin L'Huillier , Ofer Lahav , Massimiliano Lattanzi , Hayden Lee , Michele Liguori , Tongyan Lin , Marilena Loverde , Mathew Madhavacheril , Kiyoshi Masui , Jeff McMahon , Matthew McQuinn , P. Daniel Meerburg , Mehrdad Mirbabayi , Pavel Motloch , Suvodip Mukherjee , Julian B. Munõz , Johanna Nagy , Laura Newburgh , Michael D. Niemack , Andrei Nomerotski , Lyman Page , Francesco Piacentni , Elena Pierpaoli , Levon Pogosian , Clement Pryke , Giuseppe Puglisi , Radek Stompor , Marco Raveri , Christian L. Reichardt , Benjamin Rose , Graziano Rossi , John Ruhl , Emmanuel Schaan , Michael Schubnell , Katelin Schutz , Neelima Sehgal , Leonardo Senatore , Hee-Jong Seo , Blake D. Sherwin , Sara Simon , Anže Slosar , Suzanne Staggs , Albert Stebbins , Aritoki Suzuki , Eric R. Switzer , Peter Timbie , Matthieu Tristram , Mark Trodden , Yu-Dai Tsai , Caterina Umiltà , Eleonora Di Valentino , M. Vargas-Magaña , Abigail Vieregg , Scott Watson , Thomas Weiler , Nathan Whitehorn , W. L. K. Wu , Weishuang Xu , Zhilei Xu , Siavash Yasini , Matias Zaldarriaga , Gong-Bo Zhao , Ningfeng Zhu , Joe Zuntz

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…

宇宙学与河外天体物理 · 物理学 2015-06-04 Keith A. Olive , Patrick Petitjean , Elisabeth Vangioni , Joseph Silk

Cosmic microwave background (CMB) determinations of the baryon-to-photon ratio $\eta \propto \Omega_{\rm baryon} h^2$ will remove the last free parameter from (standard) big bang nucleosynthesis (BBN) calculations. This will make BBN a much…

天体物理学 · 物理学 2008-11-26 Richard H. Cyburt , Brian D. Fields , Keith A. Olive

Primordial or big bang nucleosynthesis (BBN) is one of the three historical strong evidences for the big bang model. The recent results by the Planck satellite mission have slightly changed the estimate of the baryonic density compared to…

宇宙学与河外天体物理 · 物理学 2015-06-19 Alain Coc , Jean-Philippe Uzan , Elisabeth Vangioni

Standard big bang nucleosynthesis (BBNS) promises accurate predictions of the primordial abundances of deuterium, helium-3, helium-4 and lithium-7 as a function of a single parameter. Previous measurements have nearly always been…

天体物理学 · 物理学 2008-02-03 Scott Burles , David Tytler

Primordial or big bang nucleosynthesis (BBN) is now a parameter free theory whose predictions are in good overall agreement with observations. However, the 7Li calculated abundance is significantly higher than the one deduced from…

宇宙学与河外天体物理 · 物理学 2017-03-20 Alain Coc

$f(R)$ gravity is one of the serious alternatives of general relativity having a large range of astronomical consequences. In this work, we study Big Bang Nucleosynthesis (BBN) in $f(R)$ gravity theory. We consider modification to gravity…

宇宙学与河外天体物理 · 物理学 2024-08-13 Abhijit Talukdar , Sanjeev Kalita

Recent confrontations of the predictions of standard big bang nucleosynthesis (SBBN) with the primordial abundances of the light nuclides inferred from observational data reveal a conflict. Simply put, compared to theoretical expectations…

天体物理学 · 物理学 2007-05-23 Gary Steigman

We consider the Big Bang Nucleosynthesis (BBN) bounds on light dark matter whose cross section off nucleons is sufficiently large to enable acceleration by scattering off of cosmic rays in the local galaxy. Such accelerated DM could then…

高能物理 - 唯象学 · 物理学 2020-07-01 Gordan Krnjaic , Samuel D. McDermott