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翻訳と辞書　辞書検索 [ 開発暫定版 ] スポンサード リンク Relativistic images ： ウィキペディア英語版 Relativistic images Relativistic images are images of gravitational lensing which result due to light deflections by angles $\backslash hat\; >\; 3\; \backslash pi/2$. This term was coined by Virbhadra and Ellis〔K. S. Virbhadra and G. F. R. Ellis, ''Phys. Rev.'' D62, 084003 (2000). 〕 in the year 2000 and is used by many researchers working in this field〔Examples: *A. Y. Bin-Nun, ''Phys. Rev.'' D 81, 123011 (2010); *O. Yu. Tsupko and G. S. Bisnovatyi-Kogan, ''Gravitation and Cosmology'', 15, 184 (2009); *E. F. Eiroa, G. E. Romero, and D. F. Torres, ''Phys. Rev.'' D66, 024010 (2002); *T. Kanti Dey, S. Sen, Mod. ''Phys. Lett.'' A23, 953 (2008); *E. F. Eiroa, ''Phys. Rev.'' D71, 083010 (2005); *V. Bozza, ''Phys. Rev.'' D67, 103006 (2003); *A. Bhadra, ''Phys.Rev.'' D67 (2003) 103009; *K. Sarkar, A. Bhadra, ''Class. Quant. Grav.'' 23 (2006) 6101; *Y. Liu, S. Chen, Jiliang Jing, ''Phys. Rev.'' D81:124017, 2010; *G. N. Gyulchev, S. S. Yazadjiev, ''Phys. Rev.'' D75, 023006,(2007); *S. Chen, J.Jing ''Phys. Rev.'' D80, 024036, (2009); *G. N. Gyulchev, S. S. Yazadjiev, ''Phys. Rev.'' D78, 083004, (2008); *A.O. Petters, ''Mon. Not .Roy. Astron. Soc.'' 338 (2003) 457; *A. S. Majumdar, N. Mukherjee, ''Int. J. Mod. Phys.'' D14 (2005) 1095; *M. Sereno, ''Phys.Rev.'' D69 (2004) 023002; *I. Zh. Stefanov, S. S. Yazadjiev, G. G. Gyulchev, arXiv:1003.1609v2 (); *N. Mukherjee, A. S. Majumdar, ''Gen. Rel. Grav.'' 39, 583, (2007); *Clarissa-Marie Claudel, K.S. Virbhadra, and G. F. R. Ellis, ''J. Math. Phys.'' 42, 818-838 (2001) *K. S. Virbhadra and G. F. R. Ellis, ''Phys. Rev.'' D65, 103004 (2002); K. S. Virbhadra, ''Phys. Rev.'' D79, 083004 (2009;) *T. Ghosh, S. Sengupta, ''Phys. Rev.'' D81, 044013,2010; *R. Whisker, ''Phys. Rev.'' D71 (2005) 064004; *S. Rahvar, A. Mehrabi, M. Dominik, arXiv:1008.1033v1 (); *C. Leiva, J. Saavedra, J. Villanueva, ''Mod. Phys. Lett.'' A24, 1443, (2009); *R. Sosnovskiy, arXiv:0806.4379v4 (); *C. R. Keeton, A. O. Petters, ''Phys. Rev.'' D73 (2006) 044024; *K. K. Nandi, Yuan-Zhong Zhang, Alexander V. Zakharov, ''Phys. Rev.'' D74 (2006) 024020; *M. Sereno, F. De Luca, ''Phys. Rev.'' D78, 023008, (2008); *F. De Paolis, A. Geralico, G. Ingrosso, A.A. Nucita, A. Qadir, ''Astron. Astrophys.'' 415 (2004) 1; *C. Stornaiolo, ''Gen. Rel. Grav.'' 34 (2002) 2089; *C.R. Keeton, A. O. Petters, ''Phys. Rev.'' D72 (2005) 104006; *T. Harko, Z. Kovács, Francisco S. N. Lobo, arXiv:0908.2874v1 (); *M. Sereno, ''Phys. Rev.'' D78, 083003,(2008); *M. Sereno, ''Phys. Rev.'' D77, 043004,(2008); *S. V. Iyer and A. O. Petters, ''Gen. Rel. Grav.'' 39, 1563,(2007); *T. Harko, Z. Kovács, F. S. N. Lobo, ''Phys. Rev.'' D80, 044021, (2009); *M. Sereno, ''Mon. Not. Roy. Astron. Soc.'' 344, 942 2003; *C. G. Boehmer, T. Harko, ''Class. Quant. Grav.'' 24, 3191,(2007); *A. N. Aliev, P. Talazan, ''Phys. Rev.'' D80, 044023 (2009); *V. Perlick, arXiv:0708.0178v1 (); *V. Bozza, arXiv:0911.2187v2 ().〕 (see also in , , and .) They further defined a term ''relativistic Einstein rings''.〔 ==Relativistic Einstein rings== Relativistic Einstein rings are ringed shaped images occurring due to light deflection $\backslash hat>2\; \backslash pi$ when the light source, the lens (the deflector), and the observer are perfectly aligned. Obviously, ''relativistic Einstein rings'' are ''relativistic images'' for the case when the source, lens, and observer are aligned. Relativistic images are very much demagnified and are extremely difficult to observe due to their poor magnifications as well as some additional problems. 抄文引用元・出典: フリー百科事典『 ウィキペディア（Wikipedia）』 ■ウィキペディアで「Relativistic images」の詳細全文を読む スポンサード リンク 翻訳と辞書 : 翻訳のためのインターネットリソース Copyright(C) kotoba.ne.jp 1997-2016. All Rights Reserved.