Indirect search for dark matter and physics beyond the standard model

dc.contributor	陳傳仁	zh_TW
dc.contributor	Chen, Chuan-Ren	en_US
dc.contributor.author	蕭又澤	zh_TW
dc.contributor.author	Knas Xiao	en_US
dc.date.accessioned	2019-09-05T02:10:29Z
dc.date.available	2017-08-10
dc.date.available	2019-09-05T02:10:29Z
dc.date.issued	2017
dc.description.abstract	無中文摘要	zh_TW
dc.description.abstract	The cosmic ray p ̄/p data from 20 to 450 GeV measured by AMS-02 can be interpreted in terms of DM. By using the GALPROP code, the propagation with DM annihilating to anti-protons is calculated based on the conventional model. The b ̄b, uu ̄ and W+W− final states are considered with different DM masses and annihilating cross-section as free parameters. To see the goodness of fit, the chi-squared test will be used. Once the best-fit parameters are found, the possibility of DM can be discussed.	en_US
dc.description.sponsorship	物理學系	zh_TW
dc.identifier	G060441030S
dc.identifier.uri	http://etds.lib.ntnu.edu.tw/cgi-bin/gs32/gsweb.cgi?o=dstdcdr&s=id=%22G060441030S%22.&%22.id.&
dc.identifier.uri	http://rportal.lib.ntnu.edu.tw:80/handle/20.500.12235/102507
dc.language	英文
dc.subject	Dark matter	zh_TW
dc.subject	Indirect search	zh_TW
dc.subject	Dark matter	en_US
dc.subject	Indirect search	en_US
dc.title	Indirect search for dark matter and physics beyond the standard model	zh_TW
dc.title	Indirect search for dark matter and physics beyond the standard model	en_US

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