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Open AccessArticle

Mirror QCD and Cosmological Constant

1
Department of Astronomy and Theoretical Physics, Lund University, SE-223 62 Lund, Sweden
2
Bogoliubov Laboratory of Theoretical Physics, Joint Institute for Nuclear Research, 141980 Dubna, Russia
*
Author to whom correspondence should be addressed.
Academic Editor: Lorenzo Iorio
Universe 2017, 3(2), 43; https://doi.org/10.3390/universe3020043
Received: 19 December 2016 / Revised: 30 April 2017 / Accepted: 2 May 2017 / Published: 8 May 2017
An analog of Quantum Chromo Dynamics (QCD) sector known as mirror QCD (mQCD) can affect the cosmological evolution due to a non-trivial contribution to the Cosmological Constant analogous to that induced by the ground state in non-perturbative QCD. In this work, we explore a plausible hypothesis for trace anomalies cancellation between the usual QCD and mQCD. Such an anomaly cancellation between the two gauge theories, if it exists in Nature, would lead to a suppression or even elimination of their contributions to the Cosmological Constant. The trace anomaly compensation condition and the form of the non-perturbative mQCD coupling constant in the infrared limit have been proposed by analysing a partial non-perturbative solution of the Einstein–Yang-Mills equations of motion. View Full-Text
Keywords: QCD vacuum; mirror QCD; cosmological constant QCD vacuum; mirror QCD; cosmological constant
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MDPI and ACS Style

Pasechnik, R.; Prokhorov, G.; Teryaev, O. Mirror QCD and Cosmological Constant. Universe 2017, 3, 43. https://doi.org/10.3390/universe3020043

AMA Style

Pasechnik R, Prokhorov G, Teryaev O. Mirror QCD and Cosmological Constant. Universe. 2017; 3(2):43. https://doi.org/10.3390/universe3020043

Chicago/Turabian Style

Pasechnik, Roman; Prokhorov, George; Teryaev, Oleg. 2017. "Mirror QCD and Cosmological Constant" Universe 3, no. 2: 43. https://doi.org/10.3390/universe3020043

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