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Searching for Supersymmetric Dark Matter The Modulation Effect Due to Caustc Rings
SEARCHING FOR SUPERSYMMETRIC DARK MATTER. THE
MODULATION EFFECT DUE TO THE CAUSTIC RINGS .
0 J. D. VERGADOS
0
0 Theoretical Physics Section, University of Ioannina, GR-45110, Greece
2 E-mail:Vergados@cc.uoi.gr
t The detection of the theoretically expected dark matter is central to particle physics
c
and cosmology. Current fashionable supersymmetric models provide a natural
O dark matter candidate which is the lightest supersymmetric particle (LSP). The
theoretically obtained event rates are usually very low or even undetectable. So
0
3 the experimentalists would like to exploit the modulation effect. In the present
paper we study a specific class of non-isothermal models involving flows of caustic
rings. We find that the modulation effect arising from such models is smaller than
1 that predicted by the isothermal models.
v
8
9 1 Introduction
5
0 In recent years the consideration of exotic dark matter has become necessary
1 in order to close the Universe 1. Recent data from the Supernova Cosmology
0 Project 2 , 3 suggest that the situation can be adequately described by a
0
/ barionic component ΩB = 0.1 along with the exotic components ΩCDM = 0.3
h and ΩΛ = 0.6 (see also Turner, these proceedings).
p
- Since this particle is expected to be very massive, mχ ≥ 30GeV , and
o
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