Novel Neutrino-Floor and Dark Matter Searches with Deformed Shell Model Calculations

<div>Comparison of the DSM nuclear form factors of the <svg height="11.6412pt" id="M534" style="vertical-align:-0.04979992pt" version="1.1" viewbox="-0.0498162 -11.5914 11.6735 11.6412" width="11.6735pt" xmlns="http://www.w3.org/2000/svg" xmlns:xlink="http://www.w3.org/1999/xlink"><g transform="matrix(.0091,0,0,-0.0091,2.179,-5.741)"><path d="M453 623H65C60 580 56 530 46 472H80C103 538 110 548 175 548H389C310 380 195 168 90 0L98 -12L175 -2C273 206 366 408 462 610L453 623Z" id="g50-56"></path></g><g transform="matrix(.0091,0,0,-0.0091,6.612,-5.741)"><path d="M389 0V32C297 38 291 46 291 118V635C234 613 175 595 109 583V556L161 554C203 552 207 547 207 497V118C207 46 201 38 110 32V0H389Z" id="g50-50"></path></g></svg>Ga and <svg height="11.6412pt" id="M535" style="vertical-align:-0.04979992pt" version="1.1" viewbox="-0.0498162 -11.5914 11.6735 11.6412" width="11.6735pt" xmlns="http://www.w3.org/2000/svg" xmlns:xlink="http://www.w3.org/1999/xlink"><g transform="matrix(.0091,0,0,-0.0091,2.179,-5.741)"><path d="M453 623H65C60 580 56 530 46 472H80C103 538 110 548 175 548H389C310 380 195 168 90 0L98 -12L175 -2C273 206 366 408 462 610L453 623Z" id="g50-56"></path></g><g transform="matrix(.0091,0,0,-0.0091,6.612,-5.741)"><path d="M290 377C321 398 342 415 358 430C378 450 389 473 389 502C389 578 329 635 238 635H237C184 635 137 610 109 578L64 515L88 493C112 529 154 573 208 573S303 542 303 482C303 409 233 370 141 341L149 308C165 313 190 319 215 319C272 319 341 283 341 193C342 98 292 43 222 43C163 43 122 72 96 94C88 101 79 100 70 94C61 87 47 73 46 60C44 47 48 37 62 23C76 10 118 -12 165 -12C238 -12 430 62 430 223C430 297 379 359 290 375V377Z" id="g50-52"></path></g></svg>Ge isotopes, obtained in the present work with the corresponding effective Helm form factors.</div>

Advances in High Energy Physics

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Figure 4

Figure 4: Novel Neutrino-Floor and Dark Matter Searches with Deformed Shell Model Calculations 