ar X iv : 0 70 4 . 04 23 v 2 [ as tr o - ph ] 1 4 A ug 2 00 7 Limits on the WIMP - nucleon interactions with CsI ( Tl ) crystal detectors

نویسندگان

  • H. S. Lee
  • H. C. Bhang
  • J. H. Choi
  • H. Dao
  • I. S. Hahn
  • M. J. Hwang
  • S. W. Jung
  • W. G. Kang
  • D. W. Kim
  • H. J. Kim
  • S. C. Kim
  • S. K. Kim
  • Y. D. Kim
  • J. W. Kwak
  • Y. J. Kwon
  • J. Lee
  • J. H. Lee
  • J. I. Lee
  • M. J. Lee
  • S. J. Lee
  • J. Li
  • X. Li
  • Y. J. Li
  • S. S. Myung
  • S. Ryu
  • J. H. So
  • Q. Yue
  • J. J. Zhu
چکیده

The Korea Invisible Mass Search (KIMS) experiment presents new limits on the WIMP-nucleon cross section using data from an exposure of 3409 kg·d taken with low-background CsI(Tl) crystals at Yangyang Underground Laboratory. The most stringent limit on the spin-dependent interaction for a pure proton case is obtained. The DAMA signal region for both spin-independent and spin-dependent interactions for the WIMP masses greater than 20 GeV/c 2 is excluded by the single experiment with crystal scintillators. The existence of dark matter has been widely supported by many astronomical observations on various scales [1][2][3]. Weakly interacting massive particles (WIMPs) are a good candidate for dark matter well motivated by cosmology and supersymmetric models [4]. The Korea Invisible Mass Search (KIMS) experiment has developed low-background CsI(Tl) crystals to detect the signals from the elastic scattering of WIMP off the nucleus [5][6][7]. Both 133 Cs and 127 I are sensitive to the spin-independent (SI) and spin-dependent (SD) interactions of WIMPs. Recently, the role of CsI in the direct search for SD WIMP for pure proton coupling has been pointed out [8]. It is worth noting that 127 I is the dominant target for the SI interactions in the DAMA experiment. The pulse shape discrimination (PSD) technique allows us to statistically separate nuclear recoil (NR) signals of WIMP interactions from the electron recoil (ER) signals due to the gamma ray background [9][10]. The KIMS experiment is located at the Yangyang Un-deground Laboratory (Y2L) at a depth of 700 m under an earth overburden. Details of the KIMS experiment and the first limit with 237 kg·d exposure data can be found in the previous publication [11]. Four low-background CsI(Tl) crystals are installed in the Y2L and operated at a temperature of T = 0 • C. Throughout the exposure period, the temperature of the detector was kept stable to within ±0.1 • C. Green-enhanced photomultiplier tubes (PMTs) are mounted at both ends of each crystal. The signals from the PMTs are amplified and recorded by a 500 MHz FADC. Each event is recorded for a period of 32 µs. Both PMTs on each crystal must have at least two photoelectrons within a 2 µs window to form an event trigger. We obtained 3409 kg·d WIMP search data TABLE I: Crystals used in this analysis and amount of data for each crystal Crystal mass (kg) data (kg·days) with four crystals, as shown in Table I. The energy …

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

ar X iv : a st ro - p h / 04 12 06 1 v 1 2 D ec 2 00 4 Sensitivity of the EDELWEISS WIMP search to spin - dependent interactions The EDELWEISS Collaboration :

The EDELWEISS collaboration is searching for WIMP dark matter using natural Ge cryogenic detectors. The whole data set of the first phase of the experiment contains 4.8 kg.day of data on Ge, the naturally present (7.8%), high-spin Ge isotope. The sensitivity of the experiment to the spin-dependent WIMP-nucleon interactions is evaluated using the model-independent framework proposed by Tovey et ...

متن کامل

New limits on interactions between weakly interacting massive particles and nucleons obtained with CsI(Tl) crystal detectors.

New limits are presented on the cross section for weakly interacting massive particle (WIMP) nucleon scattering in the KIMS CsI(Tℓ) detector array at the Yangyang Underground Laboratory. The exposure used for these results is 24 524.3  kg·days. Nuclei recoiling from WIMP interactions are identified by a pulse shape discrimination method. A low energy background due to alpha emitters on the crys...

متن کامل

ar X iv : 0 70 8 . 19 35 v 1 [ as tr o - ph ] 1 4 A ug 2 00 7 Testing modified gravity with globular cluster velocity dispersions

Globular clusters in the Milky Way have characteristic velocity dispersions that are consistent with the predictions of Newtonian gravity, and may be at odds with Modified Newtonian Dynamics (MOND) and possibly the cold dark matter model. We discuss a modified gravity (MOG) theory that can successfully model the velocity dispersions of GCs in the Galactic neighborhood. MOG produces velocity dis...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2008