Non-Thermal Corrections to Hawking Radiation Versus the Information Paradox**
نویسندگان
چکیده
منابع مشابه
Non-Thermal Corrections to Hawking Radiation Versus the Information Paradox
We provide a model-independent argument indicating that for a black hole of entropy N the non-thermal deviations from Hawking radiation, per each emission time, are of order 1/N , as opposed to e−N . This fact abolishes the standard a priory basis for the information paradox. Based on discussion given at 2015 Erice Summer School ”Future of Our Physics Including New Frontiers.” The famous Hawkin...
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The QCD counterpart of Hawking radiation from black holes leads to thermal hadron production in high energy collisions, from e+e− annihilation to heavy ion interactions. This hadronic radiation is formed by tunnelling through the event horizon of colour confinement and is emitted at a universal temperature TH ≃ (σ/2π)1/2, where σ denotes the string tension. Since the event horizon does not allo...
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We conjecture that because of color confinement, the physical vacuum forms an event horizon for quarks and gluons which can be crossed only by quantum tunneling, i.e., through the QCD counterpart of Hawking radiation by black holes. Since such radiation cannot transmit information to the outside, it must be thermal, of a temperature determined by the chromodynamic force at the confinement surfa...
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ژورنال
عنوان ژورنال: Fortschritte der Physik
سال: 2016
ISSN: 0015-8208
DOI: 10.1002/prop.201500096