Detecting dark energy in long baseline neutrino oscillations

GU Pei-Hong; BI Xiao-Jun; FENG Bo; YOUNG Bing-Lin; ZHANG Xin-Min

doi:10.1088/1674-1137/32/7/004

Chinese Physics C> 2008, Vol. 32> Issue(7) : 530-535 DOI: 10.1088/1674-1137/32/7/004

Detecting dark energy in long baseline neutrino oscillations

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Abstract：
In this paper, we discuss a possibility of studying properties of dark energy in long baseline neutrino oscillation experiments. We consider two types of models of neutrino dark energy. For one type of models the scalar field is taken to be quintessence-like and for the other phantom-like. In these models the scalar fields couple to the neutrinos to give rise to spatially varying neutrino masses. We will show that the two types of models predict different behaviors of the spatial variation of the neutrino masses inside the Earth and consequently result in different signals in long baseline neutrino oscillation experiments.

References

[1]

. Pelmutter S et al. Astrophys. J., 1997, 483: 5652. Spergel D N et al. Astrophys. J. Suppl., 2003, 148: 1753. Tegmark M et al. (SDSS Collaboration). Phys. Rev. D,2004, 69: 1035014. McDonald P et al. Mon. Not. Roy. Astron. Soc., 2005, 360:14715. Wetterich C. Nucl. Phys. B, 1998, 302: 6686. Ratra B, Peebles P J E. Phys. Rev. D, 1998, 37: 34067. Frieman J A. Hill C T, Stebbins A, Waga I. Phys. Rev.Lett., 1995, 75: 20778. Zlatev I, WANG L, Steinhardt P J. Phys. Rev. Lett., 1999,82: 8969. Steinhardt P J, WANG L, Zlatev I. Phys. Rev. D, 1999,59: 12350410. Armendariz-Picon C, Mukhanov V, Steinhardt P J. Phys.Rev. Lett., 2000, 85: 443811. Armendariz-Picon C, Mukhanov V, Steinhardt P J. Phys.Rev. D, 2001, 63: 10351012. Chiba T, Okabe T, Yamaguchi M. Phys. Rev. D, 2000, 62:02351113. Caldwell R R. Phys. Lett. B, 2002, 545: 2314. FENG B, WANG X, ZHANG X. Phys. Lett. B, 2005, 607:3515. GUO Z K, PIAO Y S, ZHANG X M, ZHANG Y Z. Phys.Lett. B, 2005, 608: 17716. FENG B, LI M, PIAO Y S, ZHANG X. Phys. Lett. B, 2006,634: 101-10517. LI M, FENG B, ZHANG X. JCAP, 2005, 0512: 00218. LI M, WANG X, FENG B, ZHANG X. Phys. Rev. D, 2002,65: 10351119. LI M, ZHANG X. Phys. Lett. B, 2003, 573: 2020. GU P, WANG X, ZHANG X. Phys. Rev. D, 2003, 69:08730121. Fardon R, Nelson A E, Weiner N. JCAP, 2004, 0410: 00522. Kaplan D B, Nelson A E, Weiner N. Phys. Rev. Lett., 2004,93: 09180123. BI X J, GU P, WANG X, ZHANG X. Phys. Rev. D, 2004,69: 11300724. GU P, BI X J. Phys. Rev. D, 2004, 70: 06351125. Peccei R D. Phys. Rev. D, 2005, 71: 02352726. LI H, DAI Z, ZHANG X. Phys. Rev. D, 2005, 71: 11300327. BI X J, FENG B, LI H, ZHANG X. Phys. Rev. D, 2005,72: 12352328. Brook eld A W, van de Bruck C, Mota D F, Tocchini-Valentini D. Phys. Rev. Lett., 2006, 96: 06130129. Horvat R. JCAP, 2006, 0601: 01530. Takahashi R, Tanimoto M. Phys. Lett. B, 2006, 633: 675-68031. Fardon R, Nelson A E, Weiner N. JHEP, 2006, 0603: 04232. Blennow M, Ohlsson T, Winter W. Eur. Phys. J. C, 2007,49: 1023-103933. Weiner N, Zurek K. Phys. Rev. D, 2006, 74: 02351734. LI H, FENG B, XIA J Q, ZHANG X. Phys. Rev. D, 2006,73: 10350335. Honda M, Takahashi R, Tanimoto M. JHEP, 2006, 0601:04236. Bauer F, Eisele M T, Garny M. Phys. Rev. D, 2006, 74:02350937. GU P, BI X J, ZHANG X. Eur. Phys. J. C, 2007, 50: 655-65938. Barger V, Huber P, Marfatia D. Phys. Rev. Lett., 2005, 95:21180239. Cirelli M, Gonzalez-garcia M C, Pena-Garay C. Nucl. Phys.B, 2005, 719: 21940. Barger V, Marfatia D, Whisnant K. Phys. Rev. D, 2006,73: 01300541. Gonzalez-Garcia M C, de Holanda P C, Zukanovich FunchalR. Phys. Rev. D, 2006, 73: 03300842. Schwetz T, Winter W. Phys. Lett. B, 2006, 633: 557-56243. Khoury J, Weltman A. Phys. Rev. Lett., 2004, 93: 17110444. Khoury J, Weltman A. Phys. Rev. D, 2004, 69: 04402645. Damour T, Polyakov A M. Nucl. Phys. B, 1994, 423: 53246. Damour T, Polyakov A M. Gen. Relativ. Gravit., 1994, 26:117147. Dziewonsky A M, Anderson D L. Phys. Earth Planet. Inter.,1981. 25: 29748. Comelli D, Pietroni M, Riotto A. Phys. Lett. B, 2003, 571:11549. Wolfenstein L. Phys. Rev. D, 1978, 17: 236950. Mikheyev S P, Smirnov A Yu. Sov. J. Nucl. Phys., 1985,42: 91351. Araki T et al. (KamLAND Collaboration). Phys. Rev.Lett., 2005, 94: 08180152. Aliu E et al. (K2K Collaboration). Phys. Rev. Lett., 2005,94: 08180253. Apollonio M et al. (CHOOZ Collaboration). Eur. Phys. J.C, 2003, 27: 33154. Barger V, Geer S, Whisnant K. Phys. Rev. D, 2000, 61:053004

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GU Pei-Hong, BI Xiao-Jun, FENG Bo, YOUNG Bing-Lin and ZHANG Xin-Min. Detecting dark energy in long baseline neutrino oscillations[J]. Chinese Physics C, 2008, 32(7): 530-535. doi: 10.1088/1674-1137/32/7/004

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Received: 2007-10-08
Revised: 2007-10-25

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沈阳化工大学材料科学与工程学院沈阳 110142

Detecting dark energy in long baseline neutrino oscillations

Corresponding author: BI Xiao-Jun,

Received Date: 2007-10-08

Accepted Date: 2007-10-25

Available Online: 2008-07-05

Abstract:

In this paper, we discuss a possibility of studying properties of dark energy in long baseline neutrino oscillation experiments. We consider two types of models of neutrino dark energy. For one type of models the scalar field is taken to be quintessence-like and for the other phantom-like. In these models the scalar fields couple to the neutrinos to give rise to spatially varying neutrino masses. We will show that the two types of models predict different behaviors of the spatial variation of the neutrino masses inside the Earth and consequently result in different signals in long baseline neutrino oscillation experiments.

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Detecting dark energy in long baseline neutrino oscillations

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