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Astrophysical probes of Dark Matter, the case of the Milky Way

2014.10.01 18:29

물리학과사무실 조회 수:72894

아래와 같이 콜로퀴움을 개최하오니 많이 참석해 주시기 바랍니다.

4시 20분부터 제1과학관 31214 e+강의실에서 다과를 준비하오니 많은 참석 부탁드립니다.

아 래

제목: Astrophysical probes of Dark Matter, the case of the Milky Way

연사: Dr. Fabio Iocco (Institute for Theoretical Physics (IFT),

Universidad Autonoma de Madrid (UAM), Spain)

일시: 2014년 10월 8일(수) 오후4:30

장소: 제1과학관 31214 첨단e+강의실

초록: After briefly reviewing the astrophysical probes of Dark Matter properties, I will concentrate on our own Galaxy, and show how a thorough analysis of existing dynamical and photometric data can bring us relevant information on a dark component of matter in the Milky Way.

The observed rotation curve, dynamical tracer 'par excellence' tracks the full gravitational potential of the Galaxy; its comparison with the baryonic only potential -inferred by observations of stars and gas in the bulge and disk- permits to extract valuable information on the missing component, its presence and distribution in our own host Galaxy.

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Colloquium <10/8(수> Astrophysical probes of Dark Matter, the case of the Milky Way

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