Published May 23, 2011 | Version v1
Journal article

QCD relics in the present-day Universe?

  • 1. Departamento de Fisica and Centro de Fisica das Interaccoes Fundamentais, Instituto Superior Tecnico, UT Lisboa, Av. Rovisco Pais, 1049-001 Lisboa (Portugal)
  • 2. Institute of Theoretical and Experimental Physics, B. Cheremushkinskaya 25, 117218 Moscow (Russian Federation)

Description

A possibility is suggested for the formation in the Universe of domains occupied by coherent-like states of strongly correlated quark-antiquark pairs. Only domains of the radius larger than 5 fm had a chance to survive over the entire history of the Universe, while the requirement of stability against the gravitational collapse restricts the maximum domain's radius to 14 km. Within the Generalised Nambu-Jona-Lasinio model, an exponential suppression with the domain's volume is found for the overlap between the macroscopic ground-state wavefunction of the quark-antiquark pairs and the QCD vacuum. This finding supports, at the microscopic level, the above arguments in favour of the stability of the domains.

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
1343
Journal Issue
1
Journal Page Range
p. 571-573
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
9. international conference on quark confinement and the hadron spectrum
Acronym
QCHS 9
Dates
30 Aug - 3 Sep 2010
Place
Madrid (Spain)

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
42107367
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
CHIRAL SYMMETRY; GRAVITATIONAL COLLAPSE; MASS; QUANTUM CHROMODYNAMICS; QUARK-ANTIQUARK INTERACTIONS; QUARKS; STABILITY; SYMMETRY BREAKING; UNIVERSE; WAVE FUNCTIONS
Descriptors DEC
FERMIONS; FIELD THEORIES; FUNCTIONS; INTERACTIONS; PARTICLE INTERACTIONS; QUANTUM FIELD THEORY; SYMMETRY

Optional Information

Notes
(c) 2011 American Institute of Physics