空間探測(cè)暗物質(zhì)簡(jiǎn)介
發(fā)布時(shí)間:2018-02-04 07:14
本文關(guān)鍵詞: 宇宙線 暗物質(zhì) 空間天文 出處:《物理》2015年11期 論文類型:期刊論文
【摘要】:宇宙線的探測(cè)分為地面探測(cè)和空間探測(cè)。地面探測(cè)測(cè)量的是高能宇宙線(大于100 Te V)在大氣中產(chǎn)生的簇射的前鋒面。由于低能宇宙線在大氣中產(chǎn)生的簇射不能到達(dá)地面,所以要探測(cè)低能的宇宙線就需要把探測(cè)器送到大氣層外部。空間探測(cè)宇宙線的優(yōu)點(diǎn)是能測(cè)量低能宇宙線,并且能區(qū)分宇宙線的種類。暗物質(zhì)間接探測(cè)就是在宇宙線中尋找暗物質(zhì)湮滅或者衰變產(chǎn)生的信號(hào),表現(xiàn)在宇宙線能譜上就是各種超出。所以需要準(zhǔn)確區(qū)分宇宙線的種類,并且精確測(cè)量宇宙線的能譜。在文章中,作者將介紹宇宙線的相關(guān)理論以及空間探測(cè)暗物質(zhì)的研究現(xiàn)狀,并詳細(xì)介紹將于2015年底發(fā)射的暗物質(zhì)粒子探測(cè)衛(wèi)星,討論其在暗物質(zhì)間接探測(cè)方面的各種優(yōu)勢(shì)。
[Abstract]:Cosmic ray detection is divided into ground detection and space detection. Ground detection measures high energy cosmic rays (> 100Te V). The front surface of a shower in the atmosphere. A shower produced in the atmosphere by low-energy cosmic rays cannot reach the surface. Therefore, to detect low-energy cosmic rays, we need to send the detectors out of the atmosphere. The advantage of space exploration cosmic rays is that they can be measured. Indirect detection of dark matter is the search for signals produced by the annihilation or decay of dark matter in cosmic rays. In the cosmic ray spectrum is a variety of excesses. Therefore, it is necessary to accurately distinguish the types of cosmic rays, and accurately measure the energy spectrum of cosmic rays. In this article. The author will introduce the related theory of cosmic ray and the research status of space detection dark matter, and introduce in detail the dark matter particle detection satellite which will be launched on end of 2015. Its advantages in indirect detection of dark matter are discussed.
【作者單位】: 中國(guó)科學(xué)院紫金山天文臺(tái)中國(guó)科學(xué)院暗物質(zhì)與空間天文重點(diǎn)實(shí)驗(yàn)室;
【基金】:國(guó)家重點(diǎn)基礎(chǔ)研究發(fā)展計(jì)劃(批準(zhǔn)號(hào):2013CB837000)資助項(xiàng)目 中國(guó)科學(xué)院戰(zhàn)略先導(dǎo)專項(xiàng)(批準(zhǔn)號(hào):XDA04040000)
【分類號(hào)】:P145.9;O572.1
【正文快照】: Detecting dark matter in spaceCHANG JinFENG Lei GUO Jian-Hua(Key Laboratory of Dark Matter and Space Astronomy,Purple Mountain Observatory,Chinses Acad-emy of Sciences,Nanjing 210008,China)1宇宙線簡(jiǎn)介奧地利科學(xué)家Victor F.Hess在1912年研究不同海拔高度的空
【參考文獻(xiàn)】
相關(guān)期刊論文 前1條
1 常進(jìn);馮磊;郭建華;范一中;;暗物質(zhì)粒子探測(cè)衛(wèi)星及鄰近的電子宇宙射線源[J];中國(guó)科學(xué):物理學(xué) 力學(xué) 天文學(xué);2015年11期
【二級(jí)參考文獻(xiàn)】
相關(guān)期刊論文 前1條
1 XIAO MengJiao;XIAO Xiang;ZHAO Li;CAO XiGuang;CHEN Xun;CHEN YunHua;CUI XiangYi;FANG DeQing;FU ChangBo;GIBONI Karl L.;GONG HaoWei;GUO GuoDong;HU Jie;HUANG XingTao;JI XiangDong;JU YongLin;LEI SiAo;LI ShaoLi;LIN Qing;LIU HuaXuan;LIU JiangLai;LIU Xiang;LORENZON Wolfgang;MA YuGang;MAO YaJun;NI KaiXuan;PUSHKIN Kirill;REN XiangXiang;SCHUBNELL Michael;SHEN ManBing;STEPHENSON Scott;TAN AnDi;TARL,
本文編號(hào):1489671
本文鏈接:http://sikaile.net/kejilunwen/tianwen/1489671.html
最近更新
教材專著