[1]UTIYAMA R. Invariant theoretical interpretation of interaction [J].Physical Review, 1956, 101: 1597-1607.[2]KIBBLE T W B. Lorentz invariance and the gravitational field [J].Journal of Mathematical Physics, 1961(2): 212-221.[3]YANG C N. Integral formalism for gauge fields [J]. Physical Review Letters, 1974, 33: 445-447.[4]ARKANI-HAMED N, CHENG H, LUTY M, et al. Universal dynamics of spontaneous Lorentz violation and a new spin-dependent inverse-square law force [J/OL]. Journal of High Energy Physics,2005: JHEP07 [2005-07-13].http://dx.doi.org/10.1088/1126-6708/2005/07/029.[5]SCHWARZ, D. J, STARKMAN G D, HUTERER D, et al. Is the low-lmicrowave background cosmic? [J]. Physical Review Letters. 2004, 93:221301.[6]HAWKING S W, ELLIS G. Large scale structure of space-time [M].Cambridge: Cambridge University Press, 1973.[7]COLEMAN S R, GLASHOW S L. High-energy tests of lorentz invariance[J]. Physical Review D, 1999, 59: 116008.[8]CILLADAY D, KOSTELECKY V A. Lorentz-violating extension of the standard model [J]. Physical Review D, 1998, 58: 116002.[9]AMELINO-CAMELIA G. Testable scenario for relativity with minimum length [J]. Physics Letters B, 2001, 510: 255-263.[10]COHEN A G, GLASHOW S L. Very special relativity [J]. Physical Review Letters, 2006, 97: 021601.[11]GIBBONS G W, GOMIS J, POPE C N. General very special relativity is finsler geometry [J]. Physical Review D, 2007, 76: 081701.[12] RAMOND P. Field Theory: A Modern Primer [M]. Colorado:Westview Press, 1997.[13] ALDROVANDI R, PEREIRA J G. Teleparallel Gravity [M].New York: Springer, 2013. |