-
6
-
-
0033130341
-
-
This hypothesis is supported by AGASA data, N. Hayashida et al., Astropart. Phys. 10, 303 (1999).
-
(1999)
Astropart. Phys.
, vol.10
, pp. 303
-
-
Hayashida, N.1
-
9
-
-
0001828155
-
-
[JETP Lett. 4, 78 (1966)].
-
(1966)
JETP Lett.
, vol.4
, pp. 78
-
-
-
10
-
-
17044370389
-
-
T. Stanev, R. Engel, A. Muecke, R.J. Protheroe, and J.P. Rachen, Phys. Rev. D 62, 093005 (2000);
-
(2000)
Phys. Rev. D
, vol.62
, pp. 093005
-
-
Stanev, T.1
Engel, R.2
Muecke, A.3
Protheroe, R.J.4
Rachen, J.P.5
-
16
-
-
85062122001
-
-
G.R. Farrar and T. Piran, astro-ph/0010370
-
G.R. Farrar and T. Piran, astro-ph/0010370.
-
-
-
-
20
-
-
0000184422
-
-
Astrophys. J. 285, 495 (1984);
-
(1984)
Astrophys. J.
, vol.285
, pp. 495
-
-
-
21
-
-
0033164039
-
-
Astropart. Phys. 11, 303 (1999);
-
(1999)
Astropart. Phys.
, vol.11
, pp. 303
-
-
-
25
-
-
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
-
27
-
-
0034890671
-
-
A. Jain, P. Jain, D.W. McKay, and J.P. Ralston, hep-ph/0011310
-
L. Anchordoqui, H. Goldberg, T. McCauley, T. Paul, S. Reucroft, and J. Swain, Phys. Rev. D ibid. 63, 124009 (2001); A. Jain, P. Jain, D.W. McKay, and J.P. Ralston, hep-ph/0011310.
-
(2001)
Phys. Rev. D
, vol.63
, pp. 124009
-
-
Anchordoqui, L.1
Goldberg, H.2
McCauley, T.3
Paul, T.4
Reucroft, S.5
Swain, J.6
-
29
-
-
0000363112
-
-
edited by D. Kieda, M. Salamon, and B. Dingus, Salt Lake City, Utah, astro-ph/9905185
-
S.J. Sciutto, in Proceedings of the 26th International Cosmic Ray Conference, edited by D. Kieda, M. Salamon, and B. Dingus, Salt Lake City, Utah, 1999, Vol. 1, p. 411, astro-ph/9905185.
-
(1999)
Proceedings of the 26th International Cosmic Ray Conference
, vol.1
, pp. 411
-
-
Sciutto, S.J.1
-
31
-
-
0141811023
-
-
26th International Cosmic Ray Conference: Invited, Rapporteur, and Highlight Papers, edited by B.L. Dingus, D.B. Kieda, and M.H. Salamon, AIP, Melville, NY
-
HiRes Collaboration, C.C.H. Jui, in 26th International Cosmic Ray Conference: Invited, Rapporteur, and Highlight Papers, edited by B.L. Dingus, D.B. Kieda, and M.H. Salamon, AIP Conf. Proc. No. 516 (AIP, Melville, NY, 2000), p. 370.
-
(2000)
AIP Conf. Proc. No. 516
, pp. 370
-
-
Jui, C.C.H.1
-
32
-
-
0001641124
-
-
Previous analyses of the highest energy Fly's Eye event are suggestive of this composition. F. Halzen, R.A. Vázquez, T. Stanev, and H.P. Vankov, Astropart. Phys. 3, 151 (1995);
-
(1995)
Astropart. Phys.
, vol.3
, pp. 151
-
-
Halzen, F.1
Vázquez, R.A.2
Stanev, T.3
Vankov, H.P.4
-
33
-
-
33847102996
-
-
L.A. Anchordoqui, M. Kirasirova, T.P. McCauley, S. Reucroft, and J.D. Swain, Phys. Lett. B 492, 237 (2000).
-
(2000)
Phys. Lett. B
, vol.492
, pp. 237
-
-
Anchordoqui, L.A.1
Kirasirova, M.2
McCauley, T.P.3
Reucroft, S.4
Swain, J.D.5
-
34
-
-
85062143882
-
-
L.A. Anchordoqui and H. Goldberg, hep-ph/0106217
-
L.A. Anchordoqui and H. Goldberg, hep-ph/0106217.
-
-
-
-
35
-
-
85062124074
-
-
T.E. Clarke, P.P. Kronberg, and H. Boehringer, astro-ph/0011281
-
T.E. Clarke, P.P. Kronberg, and H. Boehringer, astro-ph/0011281.
-
-
-
-
36
-
-
0034689810
-
-
20 eV. Note that this implies a slight (yet unobserved) correlation between the arrival directions and the galactic center. P. Blasi, R.I. Epstein, and A.V. Olinto, Astrophys. J. Lett. 533, L123 (2000).
-
(2000)
Astrophys. J. Lett.
, vol.533
-
-
Blasi, P.1
Epstein, R.I.2
Olinto, A.V.3
-
38
-
-
4243339699
-
-
T.M. Heckman, L. Armus, and G.K. Miley, Astrophys. J., Suppl. Ser. 74, 833 (1990).
-
(1990)
Astrophys. J., Suppl. Ser.
, vol.74
, pp. 833
-
-
Heckman, T.M.1
Armus, L.2
Miley, G.K.3
-
41
-
-
0141911727
-
-
C.W. Engelbracht, M.J. Rieke, G.H. Rieke, D.M. Kelly, and J.M. Achtermann, Astrophys. J. 505, 639 (1998).
-
(1998)
Astrophys. J.
, vol.505
, pp. 639
-
-
Engelbracht, C.W.1
Rieke, M.J.2
Rieke, G.H.3
Kelly, D.M.4
Achtermann, J.M.5
-
42
-
-
85062139745
-
-
R. de Grijs, R.W. O'Connell, and J.S. Gallagher III, astro-ph/9903188; astro-ph/0010046
-
R. de Grijs, R.W. O'Connell, and J.S. Gallagher III, astro-ph/9903188; astro-ph/0010046.
-
-
-
-
43
-
-
21344460427
-
-
T.A.D. Paglione, A.P. Marscher, J.M. Jackson, and D.L. Bertsch, Astrophys. J. 460, 295 (1996).
-
(1996)
Astrophys. J.
, vol.460
, pp. 295
-
-
Paglione, T.A.D.1
Marscher, A.P.2
Jackson, J.M.3
Bertsch, D.L.4
-
47
-
-
0001687730
-
-
L.A. Anchordoqui, M.T. Dova, L.N. Epele, and J.D. Swain, Phys. Rev. D 57, 7103 (1998).
-
(1998)
Phys. Rev. D
, vol.57
, pp. 7103
-
-
Anchordoqui, L.A.1
Dova, M.T.2
Epele, L.N.3
Swain, J.D.4
-
48
-
-
85062132808
-
-
Ph.D. thesis, UNLP, Argentina, summary electronically available from astro-ph/9812445
-
15 s, the average values Ā(t) of disintegration histories obtained using Monte Carlo simulations are in very good agreement with the analytic approximation given by Eq. (12). (L. A. Anchordoqui, Ph.D. thesis, UNLP, Argentina, 1998, summary electronically available from astro-ph/9812445.) Deviations from Eq. (11) arise because the actual dependence of the photodisintegration cross section on A has a nonmonotonic variation across the Periodic Table. However, fluctuations due to the different disintegration histories are larger. The latter lead to a spread in A of the order of 10%. For details, see Ref. [7].
-
(1998)
-
-
Anchordoqui, L.A.1
-
52
-
-
0000534587
-
-
[JETP Lett. 69, 650 (1999)]. Within the uncertainties of angular resolution, the arrival direction of this event coincides with Fly's Eye event.
-
(1999)
JETP Lett.
, vol.69
, pp. 650
-
-
-
53
-
-
0000292128
-
-
The latter depends on the exact distance to the sources. The location of NGC 253 is still subject to large uncertainties. See T.J. Davidge and C.J. Pritchet, Astron. J. 100, 102 (1990), and references therein.
-
(1990)
Astron. J.
, vol.100
, pp. 102
-
-
Davidge, T.J.1
Pritchet, C.J.2
-
54
-
-
0001586114
-
-
This expression can be easily obtained by using the formalism sketched in L.A. Anchordoqui, M.T. Dova, L.N. Epele, and J.D. Swain, Phys. Rev. D 55, 7356 (1997), with a constant Γ during propagation. See [28] for details.
-
(1997)
Phys. Rev. D
, vol.55
, pp. 7356
-
-
Anchordoqui, L.A.1
Dova, M.T.2
Epele, L.N.3
Swain, J.D.4
-
56
-
-
0242301796
-
-
19.5 eV) suffer statistically significant deflections in the galactic magnetic field, T. Stanev, Astrophys. J. 479, 290 (1997).
-
(1997)
Astrophys. J.
, vol.479
, pp. 290
-
-
Stanev, T.1
-
57
-
-
0033192151
-
-
M. Takeda astro-ph/9902239
-
N. Hayashida et al., Astrophys. J. 522, 225 (1999); M. Takeda astro-ph/9902239;
-
(1999)
Astrophys. J.
, vol.522
, pp. 225
-
-
Hayashida, N.1
-
58
-
-
0001628425
-
-
Y. Uchihori, M. Nagano, M. Takeda, M. Teshima, J. Lloyd-Evans, and A.A. Watson, Astropart. Phys. 13, 151 (2000);
-
(2000)
Astropart. Phys.
, vol.13
, pp. 151
-
-
Uchihori, Y.1
Nagano, M.2
Takeda, M.3
Teshima, M.4
Lloyd-Evans, J.5
Watson, A.A.6
-
59
-
-
85062141985
-
-
P.G. Tinyakov and I.I. Tkachev, astro-ph/0102101; L.A. Anchordoqui, H. Goldberg, S. Reucroft, G.E. Romero, J. Swain, and D.F. Torres, astro-ph/0106501
-
P.G. Tinyakov and I.I. Tkachev, astro-ph/0102101; L.A. Anchordoqui, H. Goldberg, S. Reucroft, G.E. Romero, J. Swain, and D.F. Torres, astro-ph/0106501.
-
-
-
-
60
-
-
85062133184
-
-
The most recent result of the AGASA Collaboration presented at Snowmass 2001, see [2]
-
The most recent result of the AGASA Collaboration presented at Snowmass 2001, see [2].
-
-
-
-
61
-
-
85062120712
-
-
M. Lemoine, G. Sigl, and P. Biermann, astro-ph/9903124
-
M. Lemoine, G. Sigl, and P. Biermann, astro-ph/9903124.
-
-
-
-
62
-
-
0000222646
-
-
See also [12]
-
N. Hayashida et al., J. Phys. G 21, 1101 (1995). See also [12].
-
(1995)
J. Phys. G
, vol.21
, pp. 1101
-
-
Hayashida, N.1
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