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Nowadays, the nonlinear optical process of spontaneous parametric down-conversion is considered as the canonical approach for creating entangled-photon pairs. We consider three pairs of entangled photons emitted by the parametric down-conversion source, and introduce a setup for evolving these photons based on linear optics, which is composed of several polarizing beam splitters, beam splitters, and half wave plates. By using the parametric down-conversion source and the setup, we carefully design an efficient scheme for preparing six-photon hyperentangled states in both the polarization and the spatial degrees of freedom. Because we use almost all possible behaviors of the three pairs of entangled photons, the present scheme is efficient for creating six-photon hyperentangled states. Next, in the regime of weak nonlinearity we design a quantum nondemolition detection to distinguish the two cases of photons in two special spatial modes. It is worth pointing out that our scheme is much easier to realize, since the strength of the nonlinearities in the process of quantum nondemolition detection can be restricted to the scalable orders of magnitude in practicality.
[1] Knill E, Laflamme R, Milburn G J 2001 Nature 409 46
[2] Pan J W, Chen Z B, Lu C Y, Weinfurter H, Zeilinger A, Zkowski M 2012 Rev. Mod. Phys. 84 777
[3] Kwiat P G, Mattle K, Weinfurter H, Zeilinger A, Sergienko A V, Shih Y 1995 Phys. Rev. Lett. 75 4337
[4] Bouwmeester D, Pan J W, Daniell M, Weinfurter H, Zeilinger A 1999 Phys. Rev. Lett. 82 1345
[5] Pan J W, Daniell M, Gasparoni S, Weihs G, Zeilinger A 2001 Phys. Rev. Lett. 86 4435
[6] Jin G S, Lin Y, Wu B 2007 Phys. Rev. A 75 054302
[7] Wang H F, Zhang S 2009 Phys. Rev. A 79 042336
[8] Kwiat P G 1997 J. Mod. Opt. 44 2173
[9] Du K, Qiao C F 2012 J. Mod. Opt. 59 611
[10] He Y Q, Ding D, Yan F L, Gao T 2015 J. Phys. B 48 055501
[11] Simon C, Pan J W 2002 Phys. Rev. Lett. 89 257901
[12] Sheng Y B, Deng F G 2010 Phys. Rev. A 82 044305
[13] Ding D, Yan F L 2013 Phys. Lett. A 377 1088
[14] Chiuri A, Greganti C, Paternostro M, Vallone G, Mataloni P 2012 Phys. Rev. Lett. 109 173604
[15] Xu X F, Bao X H, Pan J W 2012 Phys. Rev. A 86 050304
[16] Horodecki R, Horodecki P, Horodecki M, Horodecki K 2009 Rev. Mod. Phys. 81 865
[17] Greenberger D M, Horne M A, Shimony A, Zeilinger A 1990 Am. J. Phys. 58 1131
[18] Yan F L, Gao T, Chitambar E 2011 Phys. Rev. A 83 022319
[19] Gao T, Yan F L, van Enk S J 2014 Phys. Rev. Lett. 112 180501
[20] Bai Y K, Xu Y F, Wang Z D 2014 Phys. Rev. Lett. 113 100503
[21] Boyd R W 1999 J. Mod. Opt. 46 367
[22] Kok P, Lee H, Dowling J P 2002 Phys. Rev. A 66 063814
[23] Munro W J, Nemoto K, Beausoleil R G, Spiller T P 2005 Phys. Rev. A 71 033819
[24] Nemoto K, Munro W J 2004 Phys. Rev. Lett. 93 250502
[25] Lin Q, He B, Bergou J A, Ren Y H 2009 Phys. Rev. A 80 042311
[26] Barrett S D, Kok P, Nemoto K, Beausoleil R G, Munro W J, Spiller T P 2005 Phys. Rev. A 71 060302
[27] Sheng Y B, Deng F G, Long G L 2010 Phys. Rev. A 82 032318
[28] Ding D, Yan F L, Gao T 2014 Sci. China: Phys. Mech. Astron. 57 2098
[29] Ding D, Yan F L, Gao T 2013 J. Opt. Soc. Am. B 30 3075
[30] Ding D, Yan F L 2013 Acta Phys. Sin. 62 100304 (in Chinese) [丁东, 闫凤利 2013 62 100304]
[31] Kok P, Munro W J, Nemoto K, Ralph T C, Dowling J P, Milburn G J 2007 Rev. Mod. Phys. 79 135
[32] Kok P 2008 Phys. Rev. A 77 013808
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[1] Knill E, Laflamme R, Milburn G J 2001 Nature 409 46
[2] Pan J W, Chen Z B, Lu C Y, Weinfurter H, Zeilinger A, Zkowski M 2012 Rev. Mod. Phys. 84 777
[3] Kwiat P G, Mattle K, Weinfurter H, Zeilinger A, Sergienko A V, Shih Y 1995 Phys. Rev. Lett. 75 4337
[4] Bouwmeester D, Pan J W, Daniell M, Weinfurter H, Zeilinger A 1999 Phys. Rev. Lett. 82 1345
[5] Pan J W, Daniell M, Gasparoni S, Weihs G, Zeilinger A 2001 Phys. Rev. Lett. 86 4435
[6] Jin G S, Lin Y, Wu B 2007 Phys. Rev. A 75 054302
[7] Wang H F, Zhang S 2009 Phys. Rev. A 79 042336
[8] Kwiat P G 1997 J. Mod. Opt. 44 2173
[9] Du K, Qiao C F 2012 J. Mod. Opt. 59 611
[10] He Y Q, Ding D, Yan F L, Gao T 2015 J. Phys. B 48 055501
[11] Simon C, Pan J W 2002 Phys. Rev. Lett. 89 257901
[12] Sheng Y B, Deng F G 2010 Phys. Rev. A 82 044305
[13] Ding D, Yan F L 2013 Phys. Lett. A 377 1088
[14] Chiuri A, Greganti C, Paternostro M, Vallone G, Mataloni P 2012 Phys. Rev. Lett. 109 173604
[15] Xu X F, Bao X H, Pan J W 2012 Phys. Rev. A 86 050304
[16] Horodecki R, Horodecki P, Horodecki M, Horodecki K 2009 Rev. Mod. Phys. 81 865
[17] Greenberger D M, Horne M A, Shimony A, Zeilinger A 1990 Am. J. Phys. 58 1131
[18] Yan F L, Gao T, Chitambar E 2011 Phys. Rev. A 83 022319
[19] Gao T, Yan F L, van Enk S J 2014 Phys. Rev. Lett. 112 180501
[20] Bai Y K, Xu Y F, Wang Z D 2014 Phys. Rev. Lett. 113 100503
[21] Boyd R W 1999 J. Mod. Opt. 46 367
[22] Kok P, Lee H, Dowling J P 2002 Phys. Rev. A 66 063814
[23] Munro W J, Nemoto K, Beausoleil R G, Spiller T P 2005 Phys. Rev. A 71 033819
[24] Nemoto K, Munro W J 2004 Phys. Rev. Lett. 93 250502
[25] Lin Q, He B, Bergou J A, Ren Y H 2009 Phys. Rev. A 80 042311
[26] Barrett S D, Kok P, Nemoto K, Beausoleil R G, Munro W J, Spiller T P 2005 Phys. Rev. A 71 060302
[27] Sheng Y B, Deng F G, Long G L 2010 Phys. Rev. A 82 032318
[28] Ding D, Yan F L, Gao T 2014 Sci. China: Phys. Mech. Astron. 57 2098
[29] Ding D, Yan F L, Gao T 2013 J. Opt. Soc. Am. B 30 3075
[30] Ding D, Yan F L 2013 Acta Phys. Sin. 62 100304 (in Chinese) [丁东, 闫凤利 2013 62 100304]
[31] Kok P, Munro W J, Nemoto K, Ralph T C, Dowling J P, Milburn G J 2007 Rev. Mod. Phys. 79 135
[32] Kok P 2008 Phys. Rev. A 77 013808
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