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TOPIC: Cosmological Phase Transitions


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RE: Cosmological Phase Transitions
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Imagine a time when the entire universe froze. According to a new model for dark energy, that is essentially what happened about 11.5 billion years ago, when the universe was a quarter of the size it is today.
The model, published online May 6 in the journal Physical Review D, was developed by Research Associate Sourish Dutta and Professor of Physics Robert Scherrer at Vanderbilt University, working with Professor of Physics Stephen Hsu and graduate student David Reeb at the University of Oregon.
A cosmological phase transition - similar to freezing - is one of the distinctive aspects of this latest effort to account for dark energy - the mysterious negative force that cosmologists now think makes up more than 70 percent of all the energy and matter in the universe and is pushing the universe apart at an ever-faster rate.
Another feature that distinguishes the new formulation is that it makes a testable prediction regarding the expansion rate of the universe. In addition, the micro-explosions created by the largest particle colliders should excite the dark energy field and these excitations could appear as exotic, never-seen-before sub-atomic particles.

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Title: Cosmological Phase Transitions
Authors: Norbert Straumann
(Version v2)

In this lecture at a school for condensed matter physicists, I begin with basic concepts and tools for investigating phase transitions in quantum field theory. The very different roles of global and gauge symmetries in phase transitions will be elucidated. Among the important applications of the basic theory the thermodynamics of the electroweak transition is treated in detail, and the implications for baryogenesis will be discussed. The status of lattice simulations of the transition from a high temperature quark-gluon plasma to confined hadronic matter with spontaneously broken chiral symmetry is also briefly reviewed. The various changes of the free energy density in cosmological phase transitions reinforce the cosmological constant problem. In the last part of the lecture I shall address this profound mystery of present day physics.

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