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

Abstract
HTML
Reference
Related

PDF

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

[1]	Hang Zhao , Yong-Feng Zhu , Cheng-Dong Fu , Dan Yu , Man-Qi Ruan . The Higgs signatures at the CEPC CDR baseline. Chinese Physics C, 2019, 43(2): 023001. doi: 10.1088/1674-1137/43/2/023001
[2]	Xue Pan , Yu-Fu Lin , Li-Zhu Chen , Ming-Mei Xu , Yuan-Fang Wu . Poisson baseline of net-charge fluctuations in relativisticheavy ion collisions. Chinese Physics C, 2018, 42(7): 074104. doi: 10.1088/1674-1137/42/7/074104
[3]	Andrea Addazi , Pietro Donà , Antonino Marcianò . Dynamical interactions of dark energy and dark matter: Yang-Mills condensate and QCD axions. Chinese Physics C, 2018, 42(7): 075102. doi: 10.1088/1674-1137/42/7/075102
[4]	Rui-Yun Guo , Jing-Fei Zhang , Xin Zhang . Exploring neutrino mass and mass hierarchy in the scenario of vacuum energy interacting with cold dark matter. Chinese Physics C, 2018, 42(9): 095103. doi: 10.1088/1674-1137/42/9/095103
[5]	Jing Xu , Ming Lu , Xin-Heng Guo , Li-Jun Hu . Effects of a reverse shock wave on neutrino oscillations in a new supernova model. Chinese Physics C, 2018, 42(11): 113103. doi: 10.1088/1674-1137/42/11/113103
[6]	Shivaramakrishna Singirala . Implications of fermionic dark matter on recent neutrino oscillation data. Chinese Physics C, 2017, 41(4): 043102. doi: 10.1088/1674-1137/41/4/043102
[7]	Yi Jiao . Improving nonlinear performance of the HEPS baseline design with a genetic algorithm. Chinese Physics C, 2016, 40(7): 077002. doi: 10.1088/1674-1137/40/7/077002
[8]	LI Zhi-Hui , TANG Jing-Yu . A CW superconducting linac as the proton driver for a medium baseline neutrino beam in China. Chinese Physics C, 2014, 38(12): 127001. doi: 10.1088/1674-1137/38/12/127001
[9]	LIU Guo-Fu , LUO Xiao-Liang , YANG Jun , LIN Cun-Bao , HU Qing-Qing , PENG Jin-Xian . Baseline drift effect on the performance of neutron and γ ray discrimination using frequency gradient analysis. Chinese Physics C, 2013, 37(6): 066201. doi: 10.1088/1674-1137/37/6/066201
[10]	LIU Jing-Jing , KANG Xiao-Ping , HE Zhong , Huai-Ren , SHI Huan-Yu , HUANG Hong-Chao , ZHONG Shan , FENG Hao , LI Chang-Wei . Gaussian modification of neutrino energy loss on strongly screening nuclides ⁵⁵Co and ⁵⁶Ni by electron capture in stellar interior. Chinese Physics C, 2011, 35(3): 243-247. doi: 10.1088/1674-1137/35/3/006
[11]	Jeong Ryeol . An approach to dark energy problem through linear invariants. Chinese Physics C, 2011, 35(3): 233-242. doi: 10.1088/1674-1137/35/3/005
[12]	LIU Jing-Jing . Bremsstrahlung neutrino energy loss for ²⁴Mg, ²⁸Si, ³²S, ⁴⁰Ca, ⁵⁶Fe in strong electron screening. Chinese Physics C, 2010, 34(2): 171-176. doi: 10.1088/1674-1137/34/2/003
[13]	LIU Jing-Jing . The competition of neutrino energy loss due to the pair, photo-, plasma process at the late stages of stellar evolution. Chinese Physics C, 2009, 33(1): 15-19. doi: 10.1088/1674-1137/33/1/004
[14]	LIU Jing-Jing . Plasma neutrino energy loss due to the axial-vector current at the late stages of stellar evolution. Chinese Physics C, 2009, 33(10): 834-837. doi: 10.1088/1674-1137/33/10/003
[15]	WANG Hai-Jun . Lorentz violation constrained by triplicity of lepton families and neutrino oscillations. Chinese Physics C, 2009, 33(6): 487-493. doi: 10.1088/1674-1137/33/6/016
[16]	LIU Jing-Jing , LUO Zhi-Quan . Neutrino energy loss by electron capture in magnetic field at the crusts of neutron stars. Chinese Physics C, 2008, 32(2): 108-111. doi: 10.1088/1674-1137/32/2/007
[17]	LIU Jing-Jing , LUO Zhi-Quan . Pair neutrino energy loss for nuclei ⁵⁶Fe at the late stages of stellar evolution. Chinese Physics C, 2008, 32(8): 617-619. doi: 10.1088/1674-1137/32/8/005
[18]	HUANG Chao-Guang , ZHANG Hai-Qing , GUO Han-Ying . A new gravitational model for dark energy. Chinese Physics C, 2008, 32(9): 687-691. doi: 10.1088/1674-1137/32/9/002
[19]	SUN Ya-Xuan , CAO Jun , LU Jin-Biao , MA Yu-Qian , WANG Yi-Fang , YANG Chang-Gen . Baseline Optimization of Reactor Neutrino Experiments. Chinese Physics C, 2005, 29(6): 543-548.
[20]	Chen Esheng . Average Yields of Long-Lived Charged Particles in High Energy e⁺e^- Anmiiilation. Chinese Physics C, 1993, 17(S1): 53-63.

Access

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

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

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

Article Metric

Article Views(1737)
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

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.

HTML

Reference (1)

Detecting dark energy in long baseline neutrino oscillations

Abstract：

References

Access

Article Metrics

Metrics

通讯作者: 陈斌, bchen63@163.com

Email This Article