MSSM Dark Matter in Light of Higgs and LUX Results

<div>LSP nonthermal relic abundance constraints (red regions) on <svg height="13.9678pt" id="M237" style="vertical-align:-4.67947pt" version="1.1" viewbox="-0.0498162 -9.28833 52.4949 13.9678" width="52.4949pt" xmlns="http://www.w3.org/2000/svg" xmlns:xlink="http://www.w3.org/1999/xlink"><g transform="matrix(.013,0,0,-0.013,0,0)"><path d="M300 -147C201 -63 143 98 143 270S200 602 300 686L282 710C136 610 70 450 70 271V270C70 89 136 -72 282 -170L300 -147Z" id="g113-41"></path><glyph.data ascent="3473" descent="-2876" horiz-adv-x="346" vert-adv-y="346"></glyph.data></g><g transform="matrix(.013,0,0,-0.013,4.498,0)"><path d="M766 88L752 113C719 83 690 64 681 64C674 64 672 74 679 103L724 292C758 436 724 448 701 448C680 448 666 442 639 429C594 407 514 350 441 252H439L447 289C476 423 450 448 419 448C398 448 379 441 355 427C307 400 234 344 162 249H160L180 324C203 409 197 448 170 448C144 448 82 413 23 349L35 321C57 343 96 374 108 374C115 374 117 371 111 341C87 227 57 112 24 -6L32 -12C53 -4 81 4 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The color codes are as in Figure <a href="../fig1/">1</a>.</div>

Advances in High Energy Physics

MSSM Dark Matter in Light of Higgs and LUX Results

Figure 7