arXiv · hep-ph/9907262
Cosmological QCD Phase Transition and Dark Matter
Abstract
We calculate the size distribution of quark nuggets, which could be formed due to first order QCD phase transition in the early universe. We find that there are a large number of stable Quark Nuggets which could be a viable candidate for cosmological dark matter.
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Abhijit Bhattacharyya, Jan-e Alam, Sourav Sarkar, Pradip Roy, Bikash Sinha, Sibaji Raha, Pijushpani Bhattacharjee. 1999-07-07. Cosmological QCD Phase Transition and Dark Matter. https://doi.org/10.1016/s0375-9474(99)85104-5
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