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Volumn 75, Issue 2, 2007, Pages

Bounds on length scales of classical spacetime foam models

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EID: 33846513360     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.75.024028     Document Type: Article
Times cited : (89)

References (54)
  • 1
    • 0000265682 scopus 로고
    • APNYA6 0003-4916 10.1016/0003-4916(57)90050-7
    • J.A. Wheeler, Ann. Phys. (N.Y.) 2, 604 (1957). APNYA6 0003-4916 10.1016/0003-4916(57)90050-7
    • (1957) Ann. Phys. (N.Y.) , vol.2 , pp. 604
    • Wheeler, J.A.1
  • 2
    • 0002137376 scopus 로고
    • edited by C.M. DeWitt and J.A. Wheeler (Benjamin, New York
    • J.A. Wheeler, in Battelle Rencontres 1967, edited by, C.M. DeWitt, and, J.A. Wheeler, (Benjamin, New York, 1968), pp. 242-307.
    • (1968) Battelle Rencontres 1967 , pp. 242-307
    • Wheeler, J.A.1
  • 3
    • 0001136219 scopus 로고
    • NUPBBO 0550-3213 10.1016/0550-3213(78)90375-9
    • S.W. Hawking, Nucl. Phys. NUPBBO 0550-3213 B144, 349 (1978). 10.1016/0550-3213(78)90375-9
    • (1978) Nucl. Phys. , vol.144 , pp. 349
    • Hawking, S.W.1
  • 4
    • 85010946675 scopus 로고
    • NUPBBO 0550-3213 10.1016/0550-3213(80)90151-0
    • S.W. Hawking, D.N. Page, and C.N. Pope, Nucl. Phys. NUPBBO 0550-3213 B170, 283 (1980). 10.1016/0550-3213(80)90151-0
    • (1980) Nucl. Phys. , vol.170 , pp. 283
    • Hawking, S.W.1    Page, D.N.2    Pope, C.N.3
  • 7
    • 36149016205 scopus 로고
    • PHRVAO 0031-899X 10.1103/PhysRev.66.163
    • H.A. Bethe, Phys. Rev. 66, 163 (1944). PHRVAO 0031-899X 10.1103/PhysRev.66.163
    • (1944) Phys. Rev. , vol.66 , pp. 163
    • Bethe, H.A.1
  • 8
    • 33646634021 scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.1.961
    • E.F. Beall, Phys. Rev. D 1, 961 (1970). PRVDAQ 0556-2821 10.1103/PhysRevD.1.961
    • (1970) Phys. Rev. D , vol.1 , pp. 961
    • Beall, E.F.1
  • 9
    • 0039325221 scopus 로고    scopus 로고
    • PYLBAJ 0370-2693 10.1016/S0370-2693(97)00638-2
    • S.R. Coleman and S.L. Glashow, Phys. Lett. B 405, 249 (1997). PYLBAJ 0370-2693 10.1016/S0370-2693(97)00638-2
    • (1997) Phys. Lett. B , vol.405 , pp. 249
    • Coleman, S.R.1    Glashow, S.L.2
  • 12
    • 0038579350 scopus 로고    scopus 로고
    • RMPHAT 0034-6861 10.1103/RevModPhys.75.559
    • P.J.E. Peebles and B. Ratra, Rev. Mod. Phys. 75, 559 (2003). RMPHAT 0034-6861 10.1103/RevModPhys.75.559
    • (2003) Rev. Mod. Phys. , vol.75 , pp. 559
    • Peebles, P.J.E.1    Ratra, B.2
  • 13
    • 33846485292 scopus 로고    scopus 로고
    • astro-ph/0603449.
    • D.N. Spergel, astro-ph/0603449.
    • Spergel, D.N.1
  • 19
    • 0027187532 scopus 로고
    • For the analogous problem of bubbly ice mentioned in the Introduction, the scattering of acoustic waves has been discussed by NIMAER 0168-9002 10.1016/0168-9002(93)91037-N
    • For the analogous problem of bubbly ice mentioned in the Introduction, the scattering of acoustic waves has been discussed by P.B. Price, Nucl. Instrum. Methods Phys. Res., Sect. A NIMAER 0168-9002 325, 346 (1993); 10.1016/0168-9002(93)91037-N
    • (1993) Nucl. Instrum. Methods Phys. Res., Sect. a , vol.325 , pp. 346
    • Price, P.B.1
  • 20
    • 33846535900 scopus 로고    scopus 로고
    • astro-ph/0506648.
    • P.B. Price astro-ph/0506648.
    • Price, P.B.1
  • 21
    • 33846539457 scopus 로고    scopus 로고
    • Incidentally, the motivation for these studies is the acoustic detection of ultrahigh-energy cosmic neutrinos by a possible extension of the IceCube optical array;
    • Incidentally, the motivation for these studies is the acoustic detection of ultrahigh-energy cosmic neutrinos by a possible extension of the IceCube optical array;
  • 22
    • 33747670820 scopus 로고    scopus 로고
    • see IMPAEF 0217-751X 10.1142/S0217751X0603374X
    • see J.A. Vandenbroucke, Int. J. Mod. Phys. A 21S1, 259 (2006). IMPAEF 0217-751X 10.1142/S0217751X0603374X
    • (2006) Int. J. Mod. Phys. a , vol.211 , pp. 259
    • Vandenbroucke, J.A.1
  • 23
    • 33846489915 scopus 로고    scopus 로고
    • Contrary to the case of protons, such cosmic neutrinos would not suffer from vacuum Cherenkov radiation (at least, at tree level) and bounds similar to 4 4 in the main text would not occur.
    • Contrary to the case of protons, such cosmic neutrinos would not suffer from vacuum Cherenkov radiation (at least, at tree level) and bounds similar to 4 4 in the main text would not occur.
  • 24
  • 27
    • 0344012101 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.68.085003
    • R. Lehnert, Phys. Rev. D 68, 085003 (2003). PRVDAQ 0556-2821 10.1103/PhysRevD.68.085003
    • (2003) Phys. Rev. D , vol.68 , pp. 085003
    • Lehnert, R.1
  • 28
    • 19944432237 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.70.125010
    • R. Lehnert and R. Potting, Phys. Rev. D 70, 125010 (2004). PRVDAQ 0556-2821 10.1103/PhysRevD.70.125010
    • (2004) Phys. Rev. D , vol.70 , pp. 125010
    • Lehnert, R.1    Potting, R.2
  • 29
    • 29544432373 scopus 로고    scopus 로고
    • NUPBBO 0550-3213 10.1016/j.nuclphysb.2005.11.001
    • C. Kaufhold and F.R. Klinkhamer, Nucl. Phys. NUPBBO 0550-3213 B734, 1 (2006). 10.1016/j.nuclphysb.2005.11.001
    • (2006) Nucl. Phys. , vol.734 , pp. 1
    • Kaufhold, C.1    Klinkhamer, F.R.2
  • 30
    • 0034600601 scopus 로고    scopus 로고
    • NUPBBO 0550-3213 10.1016/S0550-3213(00)00117-6
    • F.R. Klinkhamer, Nucl. Phys. NUPBBO 0550-3213 B578, 277 (2000). 10.1016/S0550-3213(00)00117-6
    • (2000) Nucl. Phys. , vol.578 , pp. 277
    • Klinkhamer, F.R.1
  • 31
    • 37649032957 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.70.045020
    • F.R. Klinkhamer and C. Rupp, Phys. Rev. D 70, 045020 (2004). PRVDAQ 0556-2821 10.1103/PhysRevD.70.045020
    • (2004) Phys. Rev. D , vol.70 , pp. 045020
    • Klinkhamer, F.R.1    Rupp, C.2
  • 32
    • 33749158559 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.72.017901
    • F.R. Klinkhamer and C. Rupp, Phys. Rev. D 72, 017901 (2005). PRVDAQ 0556-2821 10.1103/PhysRevD.72.017901
    • (2005) Phys. Rev. D , vol.72 , pp. 017901
    • Klinkhamer, F.R.1    Rupp, C.2
  • 34
    • 33846522609 scopus 로고    scopus 로고
    • The results of the present article are more general than those of Refs. on two counts. First, the results obtained here hold for the pure photon sector (which may or may not have chiral couplings to massless fermions), whereas the results of Refs. hold only for chiral gauge theory. Second, the τ=2 spacetime foam model leads to modified photon propagation by boundary-condition effects for the vacuum Maxwell equations (Sec. 2), whereas there are no anomalous effects on gauge-boson propagation in chiral gauge theory (the reason being that the τ=2 space is simply connected, as mentioned in the last paragraph of Sec. 2).
    • The results of the present article are more general than those of Refs. on two counts. First, the results obtained here hold for the pure photon sector (which may or may not have chiral couplings to massless fermions), whereas the results of Refs. hold only for chiral gauge theory. Second, the τ=2 spacetime foam model leads to modified photon propagation by boundary-condition effects for the vacuum Maxwell equations (Sec. 2), whereas there are no anomalous effects on gauge-boson propagation in chiral gauge theory (the reason being that the τ=2 space is simply connected, as mentioned in the last paragraph of Sec. 2).
  • 38
    • 16044368160 scopus 로고    scopus 로고
    • NATUAS 0028-0836 10.1038/383319a0
    • J.A. Gaidos, Nature (London) NATUAS 0028-0836 383, 319 (1996). 10.1038/383319a0
    • (1996) Nature (London) , vol.383 , pp. 319
    • Gaidos, J.A.1
  • 39
    • 14944378638 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.83.2108
    • S.D. Biller, Phys. Rev. Lett. 83, 2108 (1999). PRLTAO 0031-9007 10.1103/PhysRevLett.83.2108
    • (1999) Phys. Rev. Lett. , vol.83 , pp. 2108
    • Biller, S.D.1
  • 40
    • 11944249183 scopus 로고
    • ASJOAB 0004-637X 10.1086/175344
    • D.J. Bird, Astrophys. J. 441, 144 (1995). ASJOAB 0004-637X 10.1086/175344
    • (1995) Astrophys. J. , vol.441 , pp. 144
    • Bird, D.J.1
  • 42
    • 84927714380 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.70.065002
    • O. Gagnon and G.D. Moore, Phys. Rev. D 70, 065002 (2004). PRVDAQ 0556-2821 10.1103/PhysRevD.70.065002
    • (2004) Phys. Rev. D , vol.70 , pp. 065002
    • Gagnon, O.1    Moore, G.D.2
  • 43
    • 34250929703 scopus 로고
    • ZEPYAA 0044-3328 10.1007/BF01328280
    • A. Friedmann, Z. Phys. 21, 326 (1924), Sec. 3; ZEPYAA 0044-3328 10.1007/BF01328280
    • (1924) Z. Phys. , vol.21 , pp. 326
    • Friedmann, A.1
  • 44
    • 0009330472 scopus 로고    scopus 로고
    • English translation in GRGVA8 0001-7701 10.1023/A:1026755309811
    • English translation in A. Friedmann Gen. Relativ. Gravit. GRGVA8 0001-7701 31, 2001 (1999). 10.1023/A:1026755309811
    • (1999) Gen. Relativ. Gravit. , vol.31 , pp. 2001
    • Friedmann, A.1
  • 45
    • 17144374559 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.59.124021
    • R. Gambini and J. Pullin, Phys. Rev. D 59, 124021 (1999). PRVDAQ 0556-2821 10.1103/PhysRevD.59.124021
    • (1999) Phys. Rev. D , vol.59 , pp. 124021
    • Gambini, R.1    Pullin, J.2
  • 47
  • 49
    • 24944520864 scopus 로고    scopus 로고
    • UFNAAG 0042-1294
    • V.A. Rubakov, Usp. Fiz. Nauk 171, 913 (2001) UFNAAG 0042-1294
    • (2001) Usp. Fiz. Nauk , vol.171 , pp. 913
    • Rubakov, V.A.1
  • 50
    • 0041837276 scopus 로고    scopus 로고
    • [PHUSEY 1063-7869 10.1070/PU2001v044n09ABEH001000
    • [V.A. Rubakov Phys. Usp. 44, 871 (2001)]. PHUSEY 1063-7869 10.1070/PU2001v044n09ABEH001000
    • (2001) Phys. Usp. , vol.44 , pp. 871
    • Rubakov, V.A.1


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