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相关论文: Big Bang Nucleosynthesis

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Results of a detailed examination of the cascade nucleosynthesis resulting from the putative hadronic decay, evaporation, or annihilation of a primordial relic during the Big Bang nucleosynthesis (BBN) era are presented. It is found that…

天体物理学 · 物理学 2009-11-10 Karsten Jedamzik

Observations of clusters and super clusters of galaxies have indicated that the Universe is more dominated by baryons than ever estimated in the homogeneous cosmological model for primordial nucleosynthesis. Recent detections of possibly…

天体物理学 · 物理学 2009-10-30 T. KAJINO , M. ORITO

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…

天体物理学 · 物理学 2007-05-23 Gary Steigman

We calculate and discuss the implications of neutrino self-interactions for the physics of weak decoupling and big bang nucleosynthesis (BBN) in the early universe. In such neutrino-sector extensions of the standard model, neutrinos may not…

宇宙学与河外天体物理 · 物理学 2020-07-22 E. Grohs , George M. Fuller , Manibrata Sen

The physics of the standard hot big bang cosmology ensures that the early Universe was a primordial nuclear reactor, synthesizing the light nuclides (D, 3He, 4He, and 7Li) in the first 20 minutes of its evolution. After an overview of…

天体物理学 · 物理学 2007-05-23 G. Steigman

We investigate the implications of the standard Big-Bang Nucleosynthesis constraint on the number of light neutrinos in the framework of the two four-neutrino schemes that are favored by the results of neutrino oscillation experiments.

高能物理 - 唯象学 · 物理学 2007-05-23 S. M. Bilenky , C. Giunti , W. Grimus , T. Schwetz

We present the Big-Bang Nucleosynthesis (BBN) simulation with a bubble universe scenario around a rotating black hole (BH) in Kerr-AdS$_5$ spacetime to explain recently updated observations of light elements such as the primordial helium…

宇宙学与河外天体物理 · 物理学 2025-03-17 Akira Dohi , Issei Koga , Kazushige Ueda

We review the current cosmological status of neutrinos, with particular emphasis on their effects on Big Bang Nucleosynthesis, Large Scale Structure of the universe and Cosmic Microwave Background Radiation measurements.

天体物理学 · 物理学 2009-11-13 Ofelia Pisanti , P. D. Serpico

The recently observed Deuterium abundance in a low- metallicity high-redshift hydrogen cloud, which is about ten times larger than that observed in the near interstellar medium, is that expected from the Standard Big Bang Nucleosynthesis…

天体物理学 · 物理学 2009-10-28 Arnon Dar

Big Bang Nucleosynthesis (BBN) offers one of the most strict evidences for the Lambda-CDM cosmology at present, as well as the Cosmic Microwave Background (CMB) radiation. In this work, our main aim is to present the outcomes of our…

宇宙学与河外天体物理 · 物理学 2014-09-10 Sibel Boran , Emre Onur Kahya

Stellar nucleosynthesis is an important nuclear physics phenomenon that is responsible for presently observed chemical elements and isotope abundances. It is also one of the corner stone hypotheses that provides basis for our understanding…

太阳与恒星天体物理 · 物理学 2012-03-09 Boris Pritychenko

We examine constraints from Big Bang nucleosynthesis on type II Randall-Sundrum brane cosmologies with both a dark radiation component and a quadratic term that depends on the 5-dimensional Planck mass, M_5. Using limits on the abundances…

天体物理学 · 物理学 2009-11-07 Jonathan D. Bratt , A. C. Gault , Robert J. Scherrer , T. P. Walker

Big-Bang nucleosynthesis (BBN) represents one of the earliest phenomena that can lead to observational constraints on the early Universe properties. It is well-known that many important mechanisms and phase transitions occurred before BBN.…

高能物理 - 唯象学 · 物理学 2018-12-03 A. Arbey , J. Ellis , F. Mahmoudi , G. Robbins

Recent observational constraints on primodial deuterium and Li7 correspond to different values of the baryon-to-photon ratio when applied to the Standard Big Bang Nucleosynthesis (SBBN) model. In this article these constraints are applied…

天体物理学 · 物理学 2007-05-23 J. F. Lara

Big-bang nucleosynthesis (BBN) probes the cosmic mass-energy density at temperatures $\sim 10$ MeV to $\sim 100$ keV. Here, we consider the effect of a cosmic matter-like species that is non-relativistic and pressureless during BBN. Such a…

宇宙学与河外天体物理 · 物理学 2024-01-18 Tsung-Han Yeh , Keith A. Olive , Brian D. Fields

We study Big Bang Nucleosynthesis (BBN) constraints on heavy QCD axions. BBN offers a powerful probe of new physics that modifies the neutron-to-proton ratio during the process, thanks to the precisely measured primordial Helium-4…

高能物理 - 唯象学 · 物理学 2026-03-11 Tae Hyun Jung , Takemichi Okui , Kohsaku Tobioka , Jiabao Wang

There is continued interest in the possibility that big bang nucleosynthesis may produce significant quantities of Be and B. In this paper we reevaluate the primordial abundances taking into account uncertainties in reactions rates. We…

天体物理学 · 物理学 2009-09-25 David Thomas

Big bang nucleosynthesis (BBN) and the cosmic microwave background (CMB) have a long history together in the standard cosmology. The general concordance between the predicted and observed light element abundances provides a direct probe of…

天体物理学 · 物理学 2009-11-10 Richard H. Cyburt

The dual origin of population II Li7, in both big bang nucleosynthesis and galactic cosmic-ray nucleosynthesis is discussed. It is argued that with additional Li6 data, stringent limits on the degree of Li7 depletion can be obtained. Li7…

天体物理学 · 物理学 2007-05-23 Keith A. Olive , Brian D. Fields

An accurate quantum three-body calculation is performed for the new type of big-bang nucleosynthesis (BBN) reactions that are catalyzed by a long-lived negatively-charged, massive leptonic particle (called X^-) such as the supersymmetric…

核理论 · 物理学 2009-08-11 Masayasu Kamimura , Yasushi Kino , Emiko Hiyama
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