Probing the structure of space-time with cosmic rays

被引:181
作者
Aloisio, R
Blasi, P
Ghia, PL
Grillo, AF
机构
[1] Univ Aquila, Dipartimento Fis, I-67100 Laquila, Italy
[2] Fermilab Natl Accelerator Lab, NASA Fermilab Astrophys Grp, Batavia, IL 60510 USA
[3] CNR, Ist Cosmogeofis, I-10133 Turin, Italy
[4] Ist Nazl Fis Nucl, Lab Nazl Gran Sasso, Laquila, Italy
[5] Ist Nazl Fis Nucl, I-10125 Turin, Italy
关键词
D O I
10.1103/PhysRevD.62.053010
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The study of the interactions of cosmic rays (CR's) with universal diffuse background radiation can provide very stringent rests of the validity of special relativity. The interactions we consider are the ones characterized by well defined energy thresholds whose energy position can be predicted on the basis of special relativity. We argue that the experimental confirmation of the existence of these thresholds can in principle put very stringent limits on the scale where special relativity and/or continuity of space-time may possibly break down.
引用
收藏
页数:7
相关论文
共 41 条
[1]  
ABUZAYYAD T, 1999, P 26 INT COSM RAY C, V3, P264
[2]  
Aharonian FA, 1999, ASTRON ASTROPHYS, V349, P11
[3]   Signatures of topological defects [J].
Berezinsky, V ;
Blasi, P ;
Vilenkin, A .
PHYSICAL REVIEW D, 1998, 58 (10)
[4]  
BERTOLAMI O, GRQC0001097
[5]   Limits to quantum gravity effects on energy dependence of the speed of light from observations of TeV flares in active galaxies [J].
Biller, SD ;
Breslin, AC ;
Buckley, J ;
Catanese, M ;
Carson, M ;
Carter-Lewis, DA ;
Cawley, MF ;
Fegan, DJ ;
Finley, JP ;
Gaidos, JA ;
Hillas, AM ;
Krennrich, F ;
Lamb, RC ;
Lessard, R ;
Masterson, C ;
McEnery, JE ;
McKernan, B ;
Moriarty, P ;
Quinn, J ;
Rose, HJ ;
Samuelson, F ;
Sembroski, G ;
Skelton, P ;
Weekes, TC .
PHYSICAL REVIEW LETTERS, 1999, 83 (11) :2108-2111
[6]  
Bogoslovsky G. Yu., 1994, FORTSCHR PHYS, V42, P143
[7]  
Bogoslovsky G. Yu., 1999, GEN RELAT GRAVIT, V31, P1565
[8]  
Camelia G. A., 1998, NATURE, V393, P763
[9]  
CAMELIA GA, 1997, INT J MOD PHYS A, V12, P607
[10]   A search for ultrahigh-energy gamma rays from egret-detected active galactic nuclei using CASA-MIA [J].
Catanese, M ;
Borione, A ;
Covault, CE ;
Cronin, JW ;
Fick, BE ;
Fortson, LF ;
Gibbs, KG ;
Glasmacher, MAK ;
Green, KD ;
Kieda, D ;
Matthews, J ;
Newport, BJ ;
Nitz, D ;
Ong, RA ;
Sinclair, D ;
vanderVelde, JC .
ASTROPHYSICAL JOURNAL, 1996, 469 (02) :572-580