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Volumn 68, Issue 10, 2003, Pages

Updated limits on TeV-scale gravity from the absence of neutrino cosmic ray showers mediated by black holes

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Indexed keywords


EID: 85038983884     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.68.104025     Document Type: Article
Times cited : (78)

References (84)
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    • K. S. Thorne, in Magic Without Magic: John Archibald Wheeler, edited by J. Klauder (Freeman, San Francisco, 1972), p. 231
    • K. S. Thorne, in Magic Without Magic: John Archibald Wheeler, edited by J. Klauder (Freeman, San Francisco, 1972), p. 231.
  • 14
    • 85038981985 scopus 로고    scopus 로고
    • R. Penrose (unpublished)
    • R. Penrose (unpublished).
  • 25
    • 0000280956 scopus 로고
    • It is noteworthy that (Formula presented) is a lower bound on the final mass of the BH which coincides with Hawking’s quasilocal mass. See S. Hawking, J. Math. Phys. 9, 598 (1968).
    • (1968) J. Math. Phys. , vol.9 , pp. 598
    • Hawking, S.1
  • 28
    • 85038996477 scopus 로고    scopus 로고
    • The validity of an impact parameter description in the semiclassical calculation can be ascertained by calculating the maximum angular momentum (Formula presented) in a given collision: for (Formula presented) one finds (Formula presented)
    • The validity of an impact parameter description in the semiclassical calculation can be ascertained by calculating the maximum angular momentum (Formula presented) in a given collision: for (Formula presented) one finds (Formula presented)
  • 29
    • 85039000071 scopus 로고    scopus 로고
    • Because of the complexity of the final state, we assume that amplitude interference effects can be ignored. This permits the cross section to be written as an integration over impact parameter. One of us (H.G.) would like to thank Scott Thomas for a discussion on this point
    • Because of the complexity of the final state, we assume that amplitude interference effects can be ignored. This permits the cross section to be written as an integration over impact parameter. One of us (H.G.) would like to thank Scott Thomas for a discussion on this point.
  • 32
    • 85038976565 scopus 로고    scopus 로고
    • hep-ph/0109202
    • For recent reviews see. e.g., G. Sigl, hep-ph/0109202;
    • Sigl, G.1
  • 35
    • 85039031986 scopus 로고    scopus 로고
    • AGASA Collaboration, S. Yoshida et al., in Proceedings of the 27th International Cosmic Ray Conference, Hamburg, Germany, 2001, Vol. 3, p. 1142
    • AGASA Collaboration, S. Yoshida et al., in Proceedings of the 27th International Cosmic Ray Conference, Hamburg, Germany, 2001, Vol. 3, p. 1142.
  • 39
    • 85038985351 scopus 로고    scopus 로고
    • G. C. Archbold, Ph.D. Thesis, University of Utah, UMI-30-54514
    • G. C. Archbold, Ph.D. Thesis, University of Utah, UMI-30-54514.
  • 48
    • 85038982002 scopus 로고    scopus 로고
    • At relevant energies (Formula presented) the mean free path for (Formula presented)-ice interaction is roughly 120 cm, whereas the charged pion decay length is about (Formula presented) where (Formula presented) is the Lorentz factor. This implies that there is a negligible probability for pion decay and so the shower cools to energies where the LPM effect is small
    • At relevant energies (Formula presented) the mean free path for (Formula presented)-ice interaction is roughly 120 cm, whereas the charged pion decay length is about (Formula presented) where (Formula presented) is the Lorentz factor. This implies that there is a negligible probability for pion decay and so the shower cools to energies where the LPM effect is small.
  • 49
    • 85039024096 scopus 로고    scopus 로고
    • astro-ph/0206371
    • I. Kravchenko, astro-ph/0206371.
    • Kravchenko, I.1
  • 50
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    • D. McKay (private communication)
    • D. McKay (private communication).
  • 54
    • 0035534441 scopus 로고    scopus 로고
    • Note that the bounds on (Formula presented) given in Fig. 33 do not depend on the shape of the extra dimension and thus are valid for both flat and warped internal dimensions. See S. B. Giddings and E. Katz, J. Math. Phys. 42, 3082 (2001);
    • (2001) J. Math. Phys. , vol.42 , pp. 3082
    • Giddings, S.B.1    Katz, E.2
  • 63
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    • hep-th/9309145
    • L. Susskind, hep-th/9309145;
    • Susskind, L.1
  • 73
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    • hep-ex/0202008
    • EOT-WASH Group Collaboration, E. G. Adelberger, hep-ex/0202008.
    • Adelberger, E.G.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.