Dark Matter and Experiments for its Identification

V.  Singh; D.  Grover; V.  Sharma; L.  Singh; M. K.  Singh; A.  Kumar; S.  Shree; N. M.  Muthu; V. S.  Subrahmanyam

doi:10.15415/jnp.2015.31014

Authors

V. Singh Department of Physics, banaras hindu university, Varanasi 221005, India
D. Grover Department of Physics, banaras hindu university, Varanasi 221005, India
V. Sharma Department of Physics, banaras hindu university, Varanasi 221005, India
L. Singh Department of Physics, banaras hindu university, Varanasi 221005, India
M. K. Singh Department of Physics, banaras hindu university, Varanasi 221005, India
A. Kumar Department of Physics, banaras hindu university, Varanasi 221005, India
S. Shree Department of Physics, banaras hindu university, Varanasi 221005, India
N. M. Muthu Department of Physics, banaras hindu university, Varanasi 221005, India
V. S. Subrahmanyam Department of Physics, banaras hindu university, Varanasi 221005, India

DOI:

https://doi.org/10.15415/jnp.2015.31014

Keywords:

Dark Matter Direct Detection, under Deep Sea water, Spherical gaseous Chamber

Abstract

After Fritz Zwicky, through various theoretical models, several dark matter events have been proposed. but none of them is yet discovered. Recent experiment shows that only around 5% of the total matters present in the whole universe are visual. Rest matter is still unknown to us by any present experimental tools. this leads that detection of dark matter is one of the very challenging & curios goal for experimental physicists. For the search of suitable dark matter candidates and for rear physics events, high Purity germanium detectors, Spherical gaseous chamber detector and few more hybrid-detectors are suitable for these purposes. We proposed that any suitable detector hosted under deep sea water will be more effective than the under ground or mountain caverns.

Downloads

Download data is not yet available.

References

Akerib et al., “First results from the LuX dark matter experiment at the Sanford underground Research Facility”

Akerib et al., “techniscal results from the surface run of the LuX dark matter experiment”. Astroparticle Physics 45, 34–43 (2013). http://dx.doi.org/10.1016/j.astropartphys.2013.02.001

C. E. Aalseth et al., Phys. Rev. Lett. 106, 131301 (2011) http://dx.doi.org/10.1103/PhysRevLett.106.131301PMid:21517370

D. S. Akerib et al., arXiv:1211.3788v2

Gaitskell, Richard J. “Direct Detection of Dark Matter”. “Annual Review of Nuclear and Particle Systems” 54:315-359 (2004). http://dx.doi.org/10.1146/annurev.nucl.54.070103.181244

H. B. Li et al., Phys. Rev. Lett. 110, 261301 (2013). http://dx.doi.org/10.1103/PhysRevLett.110.113902

H. Kraus et al. ‘euReCA – the european future of cryogenic dark matter searches’ Journal of Physics: Conference Series 39, 139-141 (2006). http://dx.doi.org/10.1088/1742-6596/39/1/031

H. Kraus et al., ‘euReCA – the european Future of Dark Matter Searches with Cryogenic Detectors’ Nuclear Physics b (Proc. Suppl.) 173, 168-171 (2007). http://dx.doi.org/10.1016/j.nuclphysbps.2007.08.043

H. T. Wong, Mod. Phys. Lett. A 23, 1431 (2008); http://dx.doi.org/10.1142/S0217984908016200

H.B. Li et al., Astroparticle Physics 56, 1–8 (2014). http://dx.doi.org/10.1016/j. astropartphys.2014.02.005

K. J. Kang, J. P. Cheng, Y. H. Chen, Y. J. Li, M. B. Shen, S.Y. Wu, and Q. Yue, J. Phys. Conf. Ser. 203, 012028 (2010); http://dx.doi.org/10.1088/1742-6596/203/1/012028

Q. Yue and H. T. Wong, J. Phys. Conf. Ser. 375, 042061 (2012). http://dx.doi.org/10.1088/1742-6596/375/1/042061

Q. Yue et al., high energy Phys. Nucl. Phys. 28, 877 (2004);h.t. Wong et al., J. Phys. Conf. Ser. 39 266 (2006). http://dx.doi.org/10.1088/1742-6596/39/1/064

R. Agnese et al., arXiv:1304.4279v2

S. T. Lin et al., Phys. Rev. D 79, 061101(R) (2009)

V. Singh et al., Journal of Nuclear Physics, Material Sciences, Radiation and Applications, 1, 37-43 (2013).

WIMP Dark Matter”, CDMSII Overview, university of California, berkeley

www.kgw-isotherm.com/downloads/

www.windows2universe.org/earth/Water/temp.html