Guey-Lin Lin, Kin-Wang Ng, Husain Athar's Astroparticle Physics: Proceedings of the First Ncts PDF

By Guey-Lin Lin, Kin-Wang Ng, Husain Athar

ISBN-10: 9812381031

ISBN-13: 9789812381033

ISBN-10: 9812776869

ISBN-13: 9789812776860

Complaints fo the 1st NCTS Workshop. includes special articles via theorists and experimentalists within the newly constructing box of astroparticle physics. a number of the themes contain: neutrinos in astroparticle physics, immense bang nucleosynthesis, string thought and cosmology.

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Additional info for Astroparticle Physics: Proceedings of the First Ncts Workshop, Kenting, Taiwan, 6-8 December 2001

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19. L. Trascatti, in Procs. of the 5th International Workshop on "Topics in Astroparticle and Underground Physics (TAUP97), Gran Sasso, Italy, 1997, ed. by A. Bottino, A. diCredico, and P. Monacelli, Nucl. Phys. B70 (Proc. 442 (1998). 20. Talk given at the International Workshop on Next Generation Nucleon Decay and Neutrino Detector (NNN99), Stony Brook, 1999, Proceedings to be published by AIP. 21. The AMANDA collaboration, Astroparticle Physics, 13, 1 (2000). 22. E. , Nature 410, 441 (2001). 23.

Other dynamical arguments estimating the density of matter are in agreement with this allotment (see ref. 4 8 for a recent review). In fact, there are many reasons why most of the dark matter must be nonbaryonic. In addition to the problems with baryonic dark matter associated with nucleosynthesis or the growth of density perturbations, it is very difficult to hide baryons. There are indeed very good constraints on the possible forms for baryonic dark matter in our galaxy. Strong cases can be made against hot gas, dust, jupiter size objects, and stellar remnants such as white dwarfs and neutron stars 4 9 .

1, for all m g = 20 — 250 GeV largely independent of t a n /? and the sign of /i. In addition, the requirement t h a t m: > m^ translates into an upper bound of about 250 GeV on the bino m a s s 5 9 ' 7 2 . By further adjusting the trilinear A and accounting for sfermion mixing this upper bound can be relaxed 6 4 and by allowing for non-zero phases in the MSSM, the upper limit can be extended to about 600 GeV 6 5 . For fixed Qh2 = 1/4, we would require sfermion masses of order 120 - 250 GeV for binos with masses in the range 20 - 250 GeV.

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Astroparticle Physics: Proceedings of the First Ncts Workshop, Kenting, Taiwan, 6-8 December 2001 by Guey-Lin Lin, Kin-Wang Ng, Husain Athar

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