Published December 1995 | Version v1
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Comment on ''Brown dwarfs, quark stars, and quark-hadron phase transition''

Creators

  • 1. Institute of Nuclear Physics, Cracow (Poland)

Description

It is shown that the cosmological quark-hadron phase transition within the Lee-Wick model with a high degree of supercooling cannot be completed. No quark stars could be produced in this scenario. (author). 2 refs

Availability note (English)

MF available from INIS under the Report Number.

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Additional details

Publishing Information

Imprint Pagination
2 p.
Report number
INP--1704/PH

INIS

Country of Publication
Poland
Country of Input or Organization
Poland
INIS RN
28022345
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Descriptors DEI
DWARF STARS; NUCLEATION; PHASE TRANSFORMATIONS; QUANTUM CHROMODYNAMICS; QUARK-HADRON INTERACTIONS; QUARKS; STAR MODELS; STARS
Descriptors DEC
FERMIONS; FIELD THEORIES; INTERACTIONS; MATHEMATICAL MODELS; PARTICLE INTERACTIONS; QUANTUM FIELD THEORY

Optional Information

Contract/Grant/Project number
KBN Grants nos. 2P-03B0-83-08 and 2P-03D0-01-09