-
1
-
-
0031542933
-
-
Recent reviews include: P. Biermann, J. Phys. G 23, 1 (1997);
-
(1997)
J. Phys. G
, vol.23
, pp. 1
-
-
Biermann, P.1
-
8
-
-
9344253230
-
-
AGASA Collaboration, M. Takeda et al., Phys. Rev. Lett. 81, 1163 (1998);
-
(1998)
Phys. Rev. Lett.
, vol.81
, pp. 1163
-
-
Takeda, M.1
-
9
-
-
4243687029
-
-
Fly's Eye Collaboration, D. J. Bird et al. Phys. Rev. Lett. ibid. 71, 3401 (1993);
-
(1993)
Phys. Rev. Lett.
, vol.71
, pp. 3401
-
-
Bird, D.J.1
-
10
-
-
12044259636
-
-
Astrophys. J. 424, 491 (1994);
-
(1994)
Astrophys. J.
, vol.424
, pp. 491
-
-
-
11
-
-
11944249183
-
-
Astrophys. J. 441, 144 (1995);
-
(1995)
Astrophys. J.
, vol.441
, pp. 144
-
-
-
12
-
-
0000652862
-
-
Haverah Park Collaboration, M. A. Lawrence, R. J. O. Reid, and A. A. Watson, J. Phys. G 17, 773 (1991);
-
(1991)
J. Phys. G
, vol.17
, pp. 773
-
-
Lawrence, M.A.1
Reid, R.J.O.2
Watson, A.A.3
-
13
-
-
0034274340
-
-
M. Ave, J. A. Hinton, R. A. Vazquez, A. A. Watson, and E. Zas, Phys. Rev. Lett. 85, 2244 (2000), http://ast.leeds.ac.uk/haverah/hav-home.shtml;
-
(2000)
Phys. Rev. Lett.
, vol.85
, pp. 2244
-
-
Ave, M.1
Hinton, J.A.2
Vazquez, R.A.3
Watson, A.A.4
Zas, E.5
-
16
-
-
33750565497
-
-
figure courtesy of T. Stanev, Proceedings of the International Workshop on Observing UltraHigh Energy Cosmic Rays from Space and Earth, Metepec, Puebla, Mexico, 2000, edited by H. Salazar, L. Villaseñor, and A. Zepeda, AIP, Melville, NY
-
T. K. Gaisser (figure courtesy of T. Stanev), in Proceedings of the International Workshop on Observing UltraHigh Energy Cosmic Rays from Space and Earth, Metepec, Puebla, Mexico, 2000, edited by H. Salazar, L. Villaseñor, and A. Zepeda, AIP Conf. Proc. No. 566 (AIP, Melville, NY, 2001).
-
(2001)
AIP Conf. Proc. No. 566
-
-
Gaisser, T.K.1
-
17
-
-
0542446522
-
-
Recent detailed explorations of the GZK cutoff include S. Lee, Phys. Rev. D 58, 043004 (1998);
-
(1998)
Phys. Rev. D
, vol.58
, pp. 043004
-
-
Lee, S.1
-
18
-
-
33750535760
-
-
A. Achterberg, Y. A. Galland, C. A. Norman, and D. B. Melrose, astro-ph/9907060
-
A. Achterberg, Y. A. Galland, C. A. Norman, and D. B. Melrose, astro-ph/9907060;
-
-
-
-
19
-
-
33750534719
-
-
T. Stanev et al., astro-ph/0003484
-
T. Stanev et al., astro-ph/0003484.
-
-
-
-
20
-
-
0442290724
-
-
P. Kronberg, Rep. Prog. Phys. 57, 325 (1994); we note, however, the surprising inference that magnetic fields within galactic clusters are of microgauss strength:
-
(1994)
Rep. Prog. Phys.
, vol.57
, pp. 325
-
-
Kronberg, P.1
-
24
-
-
33750548781
-
-
E. Boldt and P. Ghosh, astro-ph/9902342
-
E. Boldt and P. Ghosh, astro-ph/9902342;
-
-
-
-
27
-
-
33750538160
-
-
E-J. Ahn, G. Medino-Tanco, P. L. Biermann, and T. Stanev, astro-ph/9911123
-
E-J. Ahn, G. Medino-Tanco, P. L. Biermann, and T. Stanev, astro-ph/9911123.
-
-
-
-
32
-
-
33750550575
-
-
S. Sarkar, hep-ph/0005256
-
S. Sarkar, hep-ph/0005256.
-
-
-
-
34
-
-
17144424263
-
-
G. Sigl, S. Lee, P. Bhattacharjee, and S. Yoshida, Phys. Rev. D 59, 043504 (1999).
-
(1999)
Phys. Rev. D
, vol.59
, pp. 043504
-
-
Sigl, G.1
Lee, S.2
Bhattacharjee, P.3
Yoshida, S.4
-
37
-
-
33750540985
-
-
M. Lemoine, G. Sigl, and P. Biermann, astro-ph/9903124
-
M. Lemoine, G. Sigl, and P. Biermann, astro-ph/9903124;
-
-
-
-
41
-
-
0000184422
-
-
Astrophys. J. 285, 495 (1984);
-
(1984)
Astrophys. J.
, vol.285
, pp. 495
-
-
-
44
-
-
2142728950
-
-
T. J. Weiler, Astrophys. 12, 379E (2000) [for corrected receipt date];
-
(2000)
Astrophys.
, vol.12
-
-
Weiler, T.J.1
-
54
-
-
0001301336
-
-
P. Jain, D. W. McKay, S. Panda, and J. P. Ralston, Phys. Lett. B 484, 267 (2000);
-
(2000)
Phys. Lett. B
, vol.484
, pp. 267
-
-
Jain, P.1
McKay, D.W.2
Panda, S.3
Ralston, J.P.4
-
55
-
-
33750539248
-
-
G. Domokos, S. KovesiDomokos, and P. T. Mikulski, hep-ph/0006328
-
G. Domokos, S. KovesiDomokos, and P. T. Mikulski, hep-ph/0006328.
-
-
-
-
57
-
-
33750548782
-
-
S. D. Wick, T. W. Kephart, T. J. Weiler, and P. L. Biermann, astro-ph/0001233
-
S. D. Wick, T. W. Kephart, T. J. Weiler, and P. L. Biermann, astro-ph/0001233.
-
-
-
-
61
-
-
33750549812
-
-
Durban, So. Africa, 1997, edited by M. S. Potgieter, B. C. Raubenheimer, and D. J. van der Walt World Scientific, Singapore
-
L. Gonzalez-Mestres, in Proceedings of the 25th ICRC, Durban, So. Africa, 1997, edited by M. S. Potgieter, B. C. Raubenheimer, and D. J. van der Walt (World Scientific, Singapore, 1997);
-
(1997)
Proceedings of the 25th ICRC
-
-
Gonzalez-Mestres, L.1
-
62
-
-
85107712938
-
-
20 eV Particles from Space, edited by J. F. Krizmanic, J. F. Ormes, and R. E. Streitmatter, AIP, Woodbury, NY
-
20 eV Particles from Space, edited by J. F. Krizmanic, J. F. Ormes, and R. E. Streitmatter, AIP Conf. Proc. No. 433 (AIP, Woodbury, NY, 1998);
-
(1998)
AIP Conf. Proc. No. 433
-
-
-
66
-
-
0034894228
-
-
G. Sigl, D. F. Torres, L. A. Anchordoqui, and G. E. Romero, Phys. Rev. D 63, 081302(R) (2001).
-
(2001)
Phys. Rev. D
, vol.63
-
-
Sigl, G.1
Torres, D.F.2
Anchordoqui, L.A.3
Romero, G.E.4
-
69
-
-
33750540728
-
-
M. Takeda et al. astro-ph/9902239
-
M. Takeda et al. astro-ph/9902239.
-
-
-
-
71
-
-
0042587026
-
-
20)yrs. (19) The correlation in energy and time becomes even more significant when it is remembered that the higher energy primary has an even higher mean energy in transit, before losses on the 2.7K background. On the other hand, certain magnetic field configurations can lead to a counterintuitive earlier arrival time for the lower energy charged primary, as shown in D. Harari, S. Mollerach, and E. Roulet, J. High Energy Phys. 02, 035 (2000).
-
(2000)
J. High Energy Phys.
, vol.2
, pp. 035
-
-
Harari, D.1
Mollerach, S.2
Roulet, E.3
-
72
-
-
33750549395
-
-
http://www-akeno.icrr.u-tokyo.ac.jp/AGASA/
-
-
-
-
73
-
-
33750564691
-
-
http://hires.physics.utah.edu
-
-
-
-
75
-
-
0033098370
-
-
Rev. Mod. Phys. 71, S165 (1999);
-
(1999)
Rev. Mod. Phys.
, vol.71
-
-
-
76
-
-
33750545951
-
-
http://www.auger.org; http:// www-lpnhep.in2p3.fr/auger/welcome.html
-
-
-
-
77
-
-
33750549599
-
-
http://www-ta.icrr.u-tokyo.ac.jp/
-
-
-
-
78
-
-
33750539677
-
-
http://ifcai.pa.cnr.it/ifcai/euso.html
-
-
-
-
79
-
-
33750565991
-
-
http://owl.gsfc.nasa.gov
-
-
-
-
80
-
-
33750570387
-
-
http://ifcai.pa.cnr.it/~sim;AirWatch/
-
-
-
-
81
-
-
33750545513
-
-
note
-
2 with respect to the horizon, e.g. HiRes, (Formula Presented) For HiRes, α∼40°N. Finally, for an orbiting experiment such as EUSO-OWL-AW, the celestial coverage is nearly 4 π sr.
-
-
-
-
82
-
-
33750553098
-
-
Private communications
-
Private communications with W. Springer and J. Belz, HiRes Collaboration members.
-
-
-
Springer, W.1
Belz, J.2
-
84
-
-
21744433950
-
-
M. Lemoine, G. Sigl, A. Olinto, and D. N. Schramm, Astrophys. J. Lett. 486, L115 (1997);
-
(1997)
Astrophys. J. Lett.
, vol.486
-
-
Lemoine, M.1
Sigl, G.2
Olinto, A.3
Schramm, D.N.4
-
90
-
-
33750538381
-
-
Blasi and Sheth [9]
-
Blasi and Sheth [9];
-
-
-
|