Possible cosmological implications of the quark-hadron phase transition

Borghini N, Cottingham WN, Mau RV (2000)
Journal of Physics G Nuclear and Particle Physics 26(6): 771-785.

Zeitschriftenaufsatz | Veröffentlicht | Englisch
 
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Autor*in
Borghini, NicolasUniBi ; Cottingham, WN; Mau, RV
Abstract / Bemerkung
We study the quark-hadron phase transition within an effective model of QCD, and find that in a reasonable range of the main parameters of the model, bodies with quark content between 10(-2) and 10 solar masses can have been formed in the early universe. In addition, we show that a significant amount of entropy is released during the transition. This may imply the existence of a higher baryon number density than is usually expected at temperatures above the QCD scale. The cosmological QCD transition may then provide a natural way of decreasing the high baryon asymmetry created by an Affleck-Dine-like mechanism down to the value required by primordial nucleosynthesis.
Erscheinungsjahr
2000
Zeitschriftentitel
Journal of Physics G Nuclear and Particle Physics
Band
26
Ausgabe
6
Seite(n)
771-785
ISSN
0954-3899
eISSN
1361-6471
Page URI
https://pub.uni-bielefeld.de/record/2375863

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Borghini N, Cottingham WN, Mau RV. Possible cosmological implications of the quark-hadron phase transition. Journal of Physics G Nuclear and Particle Physics. 2000;26(6):771-785.
Borghini, N., Cottingham, W. N., & Mau, R. V. (2000). Possible cosmological implications of the quark-hadron phase transition. Journal of Physics G Nuclear and Particle Physics, 26(6), 771-785. https://doi.org/10.1088/0954-3899/26/6/302
Borghini, Nicolas, Cottingham, WN, and Mau, RV. 2000. “Possible cosmological implications of the quark-hadron phase transition”. Journal of Physics G Nuclear and Particle Physics 26 (6): 771-785.
Borghini, N., Cottingham, W. N., and Mau, R. V. (2000). Possible cosmological implications of the quark-hadron phase transition. Journal of Physics G Nuclear and Particle Physics 26, 771-785.
Borghini, N., Cottingham, W.N., & Mau, R.V., 2000. Possible cosmological implications of the quark-hadron phase transition. Journal of Physics G Nuclear and Particle Physics, 26(6), p 771-785.
N. Borghini, W.N. Cottingham, and R.V. Mau, “Possible cosmological implications of the quark-hadron phase transition”, Journal of Physics G Nuclear and Particle Physics, vol. 26, 2000, pp. 771-785.
Borghini, N., Cottingham, W.N., Mau, R.V.: Possible cosmological implications of the quark-hadron phase transition. Journal of Physics G Nuclear and Particle Physics. 26, 771-785 (2000).
Borghini, Nicolas, Cottingham, WN, and Mau, RV. “Possible cosmological implications of the quark-hadron phase transition”. Journal of Physics G Nuclear and Particle Physics 26.6 (2000): 771-785.
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arXiv: hep-ph/0001284

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