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Quark-Hadron Phase Transition of a Hot and a Cold Universe
並列摘要
Based on the nontopological soliton model, we discuss the quark-hadron phase transition of the early Universe. In particular, we explore the possibility that the early Universe is a cold universe filled with very dense and degenerate baryons. This cold universe is then reheated by the latent heat released from the quark-hadron phase transition. We find that a typical potential in the model would dilute the dense baryons to an acceptable baryon asymmetry of the Universe. We also discuss the generation of density fluctuations during the phase transition in the cold universe.
並列關鍵字
無資料被引用紀錄
Ou, Y. I. (2010). 從平衡到改變：論娥蘇拉‧勒瑰恩《地海六部曲》之龍的演變 [master's thesis, National Taiwan Normal University]. Airiti Library. https://www.airitilibrary.com/Article/Detail?DocID=U0021-1610201315190019
延伸閱讀
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