Further results on the WIMP annual modulation signature by DAMA/NaI

被引：0

作者：

Bernabei, R

Belli, P

Cappella, F

Montecchia, F ^{[1
]}

Nozzoli, F

Incicchitti, A

Prosperi, D

Cerulli, R

Dai, CJ

Kuang, HH

Ma, JM

Ye, Z

机构：

[1] Univ Roma Tor Vergata, Dipartimento Fis, I-00133 Rome, Italy

[2] Ist Nazl Fis Nucl, Sez Roma 2, I-00133 Rome, Italy

[3] Univ Roma La Sapienza, I-00185 Rome, Italy

[4] Ist Nazl Fis Nucl, Lab Nazl Gran Sasso, I-67010 Assergi, Aq, Italy

[5] Chinese Acad, IHEP, Beijing 100039, Peoples R China

[6] Univ Zhao Quing, Quang Dong, Peoples R China

来源：

NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS | 2005年 / 138卷

关键词：

D O I：

10.1016/j.nuclphysbps.2004.11.009

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

The similar or equal to 100 kg highly radiopure NaI(TI) set-up of the DAMA project (DAMA/NaI) has investigated the model- independent WIMP annual modulation signature over seven annual cycles for a total exposure of 107731 kg x day, obtaining a model- independent evidence for the presence of a dark matter particle component in the galactic halo at 6.3 sigma C.L.. Some of the many possible corollary model-dependent quests for the candidate particle have be m investigated with the total exposure as well.

引用

页码：45 / 47

页数：3

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