On superdense superstring gases: A heretic string model approach |
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| Affiliation: | 1. Rehabilitation Studies Unit, Kolling Institute, University of Sydney, NSW 2065, Australia;2. Lead, Occupational Health and Safety Research Program, Institute of Safety, Compensation, Rehabilitation and Recovery Research, Level 11, 499 St Kilda Road, Melbourne, VIC 3004, Australia;1. Department of Physics, University of Illinois, 845 W Taylor Street, Chicago, IL 60607, USA;2. Jet Propulsion Laboratory, 4800 Oak Grove Dr, M/S 298, Pasadena, CA 91109, USA;3. TAPIR, California Institute of Technology, MC 350-17, Pasadena, CA 91125, USA;1. Institute of Nuclear Physics Polish Academy of Sciences, PL-31342 Krakow, Poland;2. Jan Kochanowski University, PL-25406 Kielce, Poland;3. GSI Helmholtzzentrum für Schwerionenforschung, D-64291 Darmstadt, Germany;4. School of Physical Sciences, National Institute of Science Education and Research, HBNI, Jatni-752050, India;5. Institute for Theoretical Physics, Goethe University, D-60438 Frankfurt am Main, Germany |
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| Abstract: | A simple model is proposed to describe a gas of free strings at very high energy density, particularly in connection with a recently discovered phase dominated by macroscopic strings. This phase appears at high energy density if open strings are forbidden. For oriented strings the probability density for strings in the energy interval (E, E + dE) is dE / E in this phase. If open strings are allowed no such phase appears. The model is compared with superstring calculations, and relevant quantities are shown to agree. The model gives a simple and intuitively appealing picture of dense, free string gases. The effective string tension is also discussed and shown to vanish at the critical temperature. |
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