The phenomenon of string spreading on the black hole horizon, as originally discussed by Susskind, is considered in the exact curved Schwarzschild background. We consider an oscillating macroscopic string encircling the black hole and contracting towards the horizon. We then compute the angular and radial spreading of the string, as seen by a static observer at spatial infinity using fixed finite resolution time. Within our case study we find that there is indeed a spreading of the string in the angular direction, such that the string eventually covers the whole horizon. However, regarding the radial direction, we find that Lorentz-contraction suppresses the radial string spreading. [S0556-2821(99)03414-1].
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BM Birla Sci Ctr, Int Inst Applicable Math & Informat Sci, Hyderabad, India
Ist Istruz Super Carlo Livi, Prato, ItalyBM Birla Sci Ctr, Int Inst Applicable Math & Informat Sci, Hyderabad, India
Corda, C.
Feleppa, F.
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Univ Utrecht, Inst Theoret Phys, Utrecht, NetherlandsBM Birla Sci Ctr, Int Inst Applicable Math & Informat Sci, Hyderabad, India
Feleppa, F.
Tamburini, F.
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Zentrum Kunst & Medien, Karlsruhe, GermanyBM Birla Sci Ctr, Int Inst Applicable Math & Informat Sci, Hyderabad, India
Tamburini, F.
Licata, I
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Inst Sci Methodol ISEM, Palermo, Italy
Sch Adv Int Studies Theoret & Nonlinear Methodol, Bari, ItalyBM Birla Sci Ctr, Int Inst Applicable Math & Informat Sci, Hyderabad, India