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dc.contributor.authorChen, Chian-Shuen_US
dc.contributor.authorLin, Yen-Hsunen_US
dc.contributor.authorLin, Guey-Linen_US
dc.date.accessioned2020-10-05T02:02:22Z-
dc.date.available2020-10-05T02:02:22Z-
dc.date.issued2016-01-01en_US
dc.identifier.isbn978-4-89027-118-4en_US
dc.identifier.urihttp://dx.doi.org/10.7566/JPSCP.14.020103en_US
dc.identifier.urihttp://hdl.handle.net/11536/155525-
dc.description.abstractThe halo dark matter (DM) can be captured by the Sun if its final velocity after the collision with a nucleus in the Sun is less than the escape velocity. We consider a selfinteracting dark matter (SIDM) model where U(1) gauge symmetry is introduced to account for the DM self-interaction. Such a model naturally leads to isospin violating DM- nucleon interaction, although isospin symmetric interaction is still allowed as a special case. We present the IceCube-PINGU 2 sigma sensitivity to the parameter range of the above model with 5 years of search for neutrino signature from DM annihilation in the Sun. This indirect detection complements the direct detection by probing those SIDM parameter ranges which are either the region for very small m(chi) or the region opened up due to isospin violations.en_US
dc.language.isoen_USen_US
dc.subjectdark matter self-interactionen_US
dc.subjecthidden U(1)en_US
dc.subjectsolar captureen_US
dc.subjectdark matter searchen_US
dc.titleComplementary Test of the Dark Matter Self-Interaction in Dark U(1) Model by Direct and Indirect Detectionen_US
dc.typeProceedings Paperen_US
dc.identifier.doi10.7566/JPSCP.14.020103en_US
dc.identifier.journalPROCEEDINGS OF THE 14TH INTERNATIONAL SYMPOSIUM ON NUCLEI IN THE COSMOS (NIC2016)en_US
dc.citation.spage0en_US
dc.citation.epage0en_US
dc.contributor.department物理研究所zh_TW
dc.contributor.departmentInstitute of Physicsen_US
dc.identifier.wosnumberWOS:000566261100073en_US
dc.citation.woscount0en_US
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