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Particle components of dark matter
Pages 53-58

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From page 53...
... Consider fast the g~ncric dependency on mass ~> of 1bc possible relic density of a '-auto" or other c~! cclro(#akI~ illlel~cling Patricia Vsutb its tb6 LSP.
From page 54...
... 1 Tom qu~dr~(c d\~0c~s in 1b~ Standard Model (~) couplings to grand united 1beo,> {O-t!
From page 55...
... Cat ~ man ~ Fig ~ ~ find (~0 %~ ~ ~ ~ ~ ~ ~ ~ O ~ ~ ~ ~ 17 ~ ~ ~ ~ O alla tall ~ ~ j.4. Tbese lower limits all tall ~ corms about l~ec~use {132 ~ 0.3 is poss~iblc ollly if age ~ 400 GeY for tarn ~ ~ 2, Roberts 1lle LOP Hangs IT its impose increasingly strong lower limits all a.
From page 56...
... TbTec major strategies far experimental searches ~r massing cold dark mailer particles sucb as 1be LSP brave been proposed. In calcuI~ting the rates far these, it is cssenti~1 to Metric+ one's attention to models~ilb an ~cccpt~le relic dressy: it does not Mae sense ~ imagine that our Grimm bate is Mae soled of ~ particles if the calculated cosmological density nab ~ 0.1.
From page 57...
... of ~uctu~bons ) ~/7 ~ the microwave background r~diatioure~indsmcoftb~discovcryofneutraIcurrC~1s.Th~t gas suggests for 11~c Weinberg~S~la~ model: COBE is su~gOst~eforinfl~don.SubsequeDby~manyoxp~rimcOts~en1 on to ~su~e sin26w very precisely, and the microwave background cxp~rim~n1s may go onto map outtb~inflaton potenli~.The downing momcntof~b~ Standard Modelrevolution Ads Be discovery of ~oj/)
From page 58...
... i8 Co~lJoquium Pack: Ellis ^ns~l~.


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