Dark matter and dark energy from quark bag model
Maxim BrilenkovDepartment of Theoretical Physics, Odessa National University, Dvoryanskaya st. 2, Odessa 65082, UkraineMaxim EingornPhysics Department, North Carolina Central University, Fayetteville st. 1801, Durham, North Carolina 27707, U.S.ALászló JenkovszkyBogolyubov Institute for Theoretical Physics, Kiev 03680, UkraineAlexander ZhukAstronomical Observatory, Odessa National University, Dvoryanskaya st. 2, Odessa 65082, Ukraine
2013en
ABI
Annotatsiya
We calculate the present expansion of our Universe endowed with relict colored objects - quarks and gluons - that survived hadronization either as isolated islands of quark-gluon "nuggets", or spread uniformly in the Universe. In the first scenario, the QNs can play the role of dark matter. In the second scenario, we demonstrate that uniform colored objects can play the role of dark energy providing the late-time accelerating expansion of the Universe.
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