Detecting dark energy in long baseline neutrino oscillations

  • 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.

  • 加载中
  • [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
  • 加载中

Get Citation
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
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 shu
Milestone
Received: 2007-10-08
Revised: 2007-10-25
Article Metric

Article Views(1739)
PDF Downloads(854)
Cited by(0)
Policy on re-use
To reuse of subscription content published by CPC, the users need to request permission from CPC, unless the content was published under an Open Access license which automatically permits that type of reuse.
通讯作者: 陈斌, bchen63@163.com
  • 1. 

    沈阳化工大学材料科学与工程学院 沈阳 110142

  1. 本站搜索
  2. 百度学术搜索
  3. 万方数据库搜索
  4. CNKI搜索

Email This Article

Title:
Email:

Detecting dark energy in long baseline neutrino oscillations

    Corresponding author: BI Xiao-Jun,

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.

    HTML

Reference (1)

目录

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return