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Books on the topic 'Big Bang Nucleosynthesis (BBN)'

Author: Grafiati

Published: 6 September 2023

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1

Hashimoto, Masa-aki, Riou Nakamura, E. P. Berni Ann Thushari, and Kenzo Arai. Big-Bang Nucleosynthesis. Singapore: Springer Singapore, 2018. http://dx.doi.org/10.1007/978-981-13-2935-7.

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2

A, Olive Keith, Fermi National Accelerator Laboratory, and United States. National Aeronautics and Space Administration., eds. Big-bang nucleosynthesis revisited. [Batavia, Ill.]: Fermi National Accelerator Laboratory, 1989.

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3

A, Olive Keith, Fermi National Accelerator Laboratory, and United States. National Aeronautics and Space Administration., eds. Big-bang nucleosynthesis revisited. [Batavia, Ill.]: Fermi National Accelerator Laboratory, 1989.

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4

Supernovae and nucleosynthesis: An investigation of the history of matter, from the big bang to the present. Princeton, N.J: Princeton University Press, 1996.

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5

1939-, Thompson William J., Carney Bruce W, and Karwowski Hugon J, eds. Workshop on Primordial Nucleosynthesis, October 6-8, 1989, Aqueduct Conference Center, Chapel Hill, North Carolina, USA. Singapore: World Scientific, 1990.

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6

(Angela), Bracco A., Nappi Eugenio, and Società italiana di fisica, eds. From the Big Bang to the nucleosynthesis: Proceedings of the International School of Physics "Enrico Fermi" Course CLXXVIII, Varenna on Lake Como, Villa Monastero, 19-24 July 2010. Amsterdam: IOS Press, 2011.

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7

Big-bang nucleosynthesis revisited. [Batavia, Ill.]: Fermi National Accelerator Laboratory, 1989.

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8

Big bang nucleosynthesis and the quark-hadron transition. [Batavia, Ill.]: Fermi National Accelerator Laboratory, 1989.

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9

Hashimoto, Masa-aki, Riou Nakamura, and E. P. Berni Ann Thushari. Big-Bang Nucleosynthesis: Thermonuclear History in the Early Universe. Springer, 2019.

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10

Hashimoto, Masa-aki, Riou Nakamura, E. P. Berni Ann Thushari, and Kenzo Arai. Big-Bang Nucleosynthesis: Thermonuclear History in the Early Universe. Springer, 2018.

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11

Deruelle, Nathalie, and Jean-Philippe Uzan. The Lambda-CDM model of the hot Big Bang. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198786399.003.0059.

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This chapter introduces the Lambda-CDM (cold dark matter) model. In 1948, under the impetus of George Gamow, Robert Hermann, Ralph Alpher, and Hans Bethe in particular, relativistic cosmology entered the second phase of its history. In this phase, physical processes, in particular, nuclear and atomic processes, are taken into account. This provides two observational tests of the model: primordial nucleosynthesis, which explains the origin of light nuclei, and the existence of the cosmic microwave background, and it establishes the fact that the universe has a thermal history. Study of the large-scale structure of the universe then indicates the existence of dark matter and a nonzero cosmological constant. This model, known as the Λ‎CDM model, is the standard model of contemporary cosmology.

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12

Arnett, David. Supernovae and Nucleosynthesis: An Investigation of the History of Matter, from the Big Bang to the Present. Princeton University Press, 2020.

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13

Thompson, William J., and Bruce W. Carney. Primordial Nucleosynthesis: Workshop October 6-8, 1989 Aqueduct Conference Center Chapel Hill, North Carolina, USA. World Scientific Pub Co Inc, 1990.

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14

Kachelriess, Michael. Thermal relics. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198802877.003.0021.

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The Boltzmann equations, which describe processes as diverse as the evolution of the dark matter density, big bang nucleosynthesis or recombination, are derived. The Gamov criterion states that processes freeze-out when their rate becomes smaller than the Hubble rate. It is demonstrated that the mass of any thermal relic is bounded by ≲ 20TeV, while the abundance of a cold dark matter particle with 〈σ‎v〉 ≃ 3 × 10−26 cm3/s corresponds to the observed one, Ω‎CDM = 0.2. Big bang nucleosynthesis, which successfully explains the abundance of light elements like D and 4He, is discussed.

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15

Close, Frank. 5. Making and breaking nuclei. Oxford University Press, 2015. http://dx.doi.org/10.1093/actrade/9780198718635.003.0005.

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‘Making and breaking nuclei’ describes the process by which the atomic elements came to be in the early universe. The heat energy in the big bang, some 13.7 billion years ago, converted into counterbalanced particles of matter and antimatter. The seeds of atomic nuclei were initially the simplest constituents: quarks. During the last 5 billion years, the majority of elements found on earth were formed inside a long-dead star, where they were all cooked from protons, which were synthesised within the first second of the universe. The processes of stellar nucleosynthesis, the CNO cycle, supernovae nucleosynthesis, and cosmic spallation are explained along with the dating of the age of the Earth.

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16

Vigdor, Steven E. Expansion Everlasting. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198814825.003.0005.

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Chapter 5 presents experiments illuminating the cosmological evolution of the universe and its energy budget, accounting for its longevity. The observations establishing the Hubble’s Law linear relationship between intergalactic distances and recession speeds, and their interpretation in terms of the expansion of cosmic space, are reviewed. The evidence for big bang cosmology from nucleosynthesis and the cosmic microwave background (CMB) is presented. The measurements that establish the ongoing acceleration of the cosmic expansion are reviewed: distant supernova recession speeds, tiny CMB anisotropies, baryon acoustic oscillations, and gravitational lensing. Excellent model fits to these data, assuming general relativity, cold dark matter, and a cosmological constant, lead to precise determinations of both the age of the universe and the energy budget of the universe. The cosmic history of the expansion rate and the energy budget are inferred, along with the remarkable flatness of cosmic space within the observable portion of the universe.

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