%Paper: 
%From: jungman@npac.syr.edu (Gerard Jungman)
%Date: Wed, 21 Jun 1995 23:59:24 -0400


% Supersymmetric Dark Matter
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\def\leaderfill{\leaders\hbox to 1em{\hss.\hss}\hfill}

\noindent
{\bf Supersymmetric Dark Matter}
\vskip 10pt

\noindent
{\it by } G. Jungman, M. Kamionkowski, and K. Griest
\vskip 10pt


\noindent {1.} {Introduction} \leaderfill{2} \par
\noindent {2.} {Dark Matter in the Universe} \leaderfill{14} \par
\noindent \quad{2.1.} {Inventory of Dark Matter} \leaderfill{14} \par
\noindent \quad{2.2.} {Theoretical arguments} \leaderfill{20} \par
\noindent \quad{2.3.} {Baryonic Content of the Universe} \leaderfill{20} \par
\noindent \quad{2.4.} {Distribution of Dark Matter in the Milky Way}
\leaderfill{22} \par
\noindent \quad{2.5.} {Overview of Dark-Matter Candidates} \leaderfill{30} \par
\noindent {3.} {Cosmological Abundance of a WIMP} \leaderfill{32} \par
\noindent \quad{3.1.} {Simple Estimates} \leaderfill{34} \par
\noindent \quad{3.2.} {Why WIMPs?} \leaderfill{38} \par
\noindent \quad{3.3.} {Standard Calculation of Relic Abundance} \leaderfill{38}
\par
\noindent \quad{3.4.} {Special Cases} \leaderfill{40} \par
\noindent \quad{3.5.} {Possible Loopholes} \leaderfill{42} \par
\noindent \quad{3.6.} {Constraints on the WIMP Density} \leaderfill{44} \par
\noindent {4.} {Supersymmetric Models} \leaderfill{46} \par
\noindent \quad{4.1.} {Motivation, Goals, and Some Formalities} \leaderfill{46}
\par
\noindent \quad{4.2.} {Minimal Supersymmetric Standard Model} \leaderfill{52}
\par
\noindent \quad{4.3.} {SUSY-GUT and Supergravity Models} \leaderfill{60} \par
\noindent {5.} {Laboratory Constraints} \leaderfill{62} \par
\noindent \quad{5.1.} {Remarks} \leaderfill{62} \par
\noindent \quad{5.2.} {Constraints on the Higgs Sector} \leaderfill{62} \par
\noindent \quad{5.3.} {Constraints on the Chargino/Neutralino Sector}
\leaderfill{64} \par
\noindent \quad{5.4.} {Sleptons} \leaderfill{64} \par
\noindent \quad{5.5.} {Squarks and Gluinos} \leaderfill{64} \par
\noindent \quad{5.6.} {Limits From Rare Processes} \leaderfill{66} \par
\noindent {6.} {Neutralino Annihilation} \leaderfill{72} \par
\noindent \quad{6.1.} {Remarks} \leaderfill{72} \par
\noindent \quad{6.2.} {Weak--Gauge-Boson Final States} \leaderfill{74} \par
\noindent \quad{6.3.} {Final States Containing Higgs Bosons} \leaderfill{78}
\par
\noindent \quad{6.4.} {Fermion Final States} \leaderfill{84} \par
\noindent \quad{6.5.} {Gluon Final States} \leaderfill{90} \par
\noindent \quad{6.6.} {Photon Final States} \leaderfill{94} \par
\noindent \quad{6.7.} {Summary of Neutralino Annihilation} \leaderfill{94} \par
\noindent {7.} {Elastic-Scattering Cross Sections} \leaderfill{96} \par
\noindent \quad{7.1.} {The Basic Ingredients} \leaderfill{96} \par
\noindent \quad{7.2.} {Axial-Vector (spin) Interaction} \leaderfill{98} \par
\noindent \quad{7.3.} {Scalar Interaction} \leaderfill{106} \par
\noindent \quad{7.4.} {General Axial-Vector, Vector, and Scalar Interactions}
\leaderfill{116} \par
\noindent \quad{7.5.} {Comparison of Spin and Scalar Cross Sections}
\leaderfill{118} \par
\noindent {8.} {Direct Detection of Neutralinos} \leaderfill{120} \par
\noindent \quad{8.1.} {Theory} \leaderfill{120} \par
\noindent \quad{8.2.} {Detectors} \leaderfill{130} \par
\noindent \quad{8.3.} {Inelastic-Scattering Techniques} \leaderfill{136} \par
\noindent {9.} {Energetic Neutrinos from WIMP Annihilation in the Sun and/or
Earth} \leaderfill{136} \par
\noindent \quad{9.1.} {General Description} \leaderfill{136} \par
\noindent \quad{9.2.} {Detectors and Atmospheric-Neutrino Background}
\leaderfill{142} \par
\noindent \quad{9.3.} {Annihilation Rate in the Sun and Earth} \leaderfill{146}
\par
\noindent \quad{9.4.} {Capture Rate in the Sun and Earth} \leaderfill{148} \par
\noindent \quad{9.5.} {Neutrino Spectra} \leaderfill{158} \par
\noindent \quad{9.6.} {Model-Independent Analysis and Summary} \leaderfill{168}
\par
\noindent \quad{9.7.} {Comparison of Direct and Indirect Detection}
\leaderfill{174} \par
\noindent {10.} {Cosmic Rays from WIMP Annihilation in the Halo}
\leaderfill{178} \par
\noindent \quad{10.1.} {Cosmic-Ray Antiprotons} \leaderfill{180} \par
\noindent \quad{10.2.} {Cosmic-Ray Positrons} \leaderfill{182} \par
\noindent \quad{10.3.} {Cosmic Gamma Rays} \leaderfill{184} \par
\noindent {11.} {Sample Analysis of the MSSM} \leaderfill{188} \par
\noindent \quad{11.1.} {Orientation} \leaderfill{188} \par
\noindent \quad{11.2.} {SUSY Parameter Space} \leaderfill{190} \par
\noindent \quad{11.3.} {Relic Density} \leaderfill{192} \par
\noindent \quad{11.4.} {Elastic Scattering Cross Sections} \leaderfill{194}
\par
\noindent \quad{11.5.} {Direct-Detection Rates} \leaderfill{196} \par
\noindent \quad{11.6.} {Indirect-Detection Rates} \leaderfill{202} \par
\noindent \quad{11.7.} {Comparison of Direct and Indirect Rates}
\leaderfill{204} \par
\noindent \quad{11.8.} {Results from Unified Models} \leaderfill{206} \par
\noindent {12.} {Other Particle Dark-Matter Candidates} \leaderfill{208} \par
\noindent \quad{12.1.} {The Rise and Fall of Heavy-Neutrino Dark Matter}
\leaderfill{210} \par
\noindent \quad{12.2.} {Sneutrinos} \leaderfill{214} \par
\noindent \quad{12.3.} {Other Supersymmetric Dark-Matter Candidates}
\leaderfill{214} \par
\noindent {13.} {Conclusions} \leaderfill{216} \par
\noindent \quad{13.1.} {Summary of Calculations} \leaderfill{218} \par
\noindent \quad{13.2.} {Central Results} \leaderfill{220} \par
\noindent \quad{13.3.} {Concluding Remarks} \leaderfill{222} \par
\noindent {14.} {Acknowledgments} \leaderfill{224} \par
\noindent Appendix {A.} {Construction of the MSSM} \leaderfill{224} \par
\noindent \quad{\hbox {A.}1.} {Introduction} \leaderfill{224} \par
\noindent \quad{\hbox {A.}2.} {Superfield Formalism} \leaderfill{224} \par
\noindent \quad{\hbox {A.}3.} {Minimal Supersymmetric Standard Model: General
Discussion} \leaderfill{226} \par
\noindent \quad{\hbox {A.}4.} {Minimal Supersymmetric Standard Model: Spectrum
and Interactions} \leaderfill{232} \par
\noindent \quad{\hbox {A.}5.} {SUSY-GUT and Supergravity Models}
\leaderfill{248} \par
\noindent \quad{\hbox {A.}6.} {Parameterizations} \leaderfill{252} \par
\noindent Appendix {B.} {User's Guide for Neutdriver} \leaderfill{254} \par

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