Starobinsky Inflation: From Non-SUSY to SUGRA Realizations

Input and output parameters of the models which are compatible with (<a href="https://static.hindawi.com/articles/ahep/volume-2017/6759267/figures/#EEq2.4">4</a>) for <svg height="15.1057pt" id="M524" style="vertical-align:-3.181499pt" version="1.1" viewbox="-0.0498162 -11.9242 52.9671 15.1057" width="52.9671pt" xmlns="http://www.w3.org/2000/svg" xmlns:xlink="http://www.w3.org/1999/xlink"><g transform="matrix(.013,0,0,-0.013,1.768,-2.897)"><path d="M658 557C549 593 437 629 340 673H318C222 629 109 593 0 557L9 532C116 551 225 577 329 602C435 576 543 551 649 532L658 557Z" id="g119-105"></path><glyph.data ascent="3473" descent="-2876" horiz-adv-x="658" vert-adv-y="658" xpluscharwidth="10.322000000000001"></glyph.data></g><g transform="matrix(.013,0,0,-0.013,0,0)"><path d="M822 650H589L583 622C660 617 677 607 674 561C672 534 664 481 647 390L600 137H596L273 650H126L120 622C176 620 194 615 207 594C221 571 225 557 214 504L161 257C141 166 129 112 121 85C108 42 83 30 29 28L23 0H260L266 28C193 33 173 42 176 89C178 122 186 172 202 255L256 527H259L583 -8H612L690 390C708 481 720 535 728 558C744 603 756 619 816 622L822 650Z" id="g113-79"></path><glyph.data ascent="3473" descent="-2876" horiz-adv-x="839" vert-adv-y="839" xpluscharwidth="10.907"></glyph.data></g><g transform="matrix(.0091,0,0,-0.0091,10.062,3.132)"><path d="M527 299L515 337L338 293L325 475H286L273 293L96 337L84 299L252 231L156 77L188 53L305 192L423 53L455 77L358 231L527 299Z" id="g50-44"></path><glyph.data ascent="3443" descent="-2856" horiz-adv-x="611" vert-adv-y="611" xpluscharwidth="15.62208167"></glyph.data></g><g transform="matrix(.013,0,0,-0.013,19.811,0)"><path d="M535 323V373H52V323H535ZM535 138V188H52V138H535Z" id="g117-34"></path><glyph.data ascent="3473" descent="-2876" horiz-adv-x="587" vert-adv-y="587" xpluscharwidth="27.442"></glyph.data></g><g transform="matrix(.013,0,0,-0.013,31.074,0)"><path d="M153 550H386L412 615L406 623H120L82 318C104 327 142 338 184 338C294 338 347 275 347 187C347 112 305 39 221 39C160 39 119 71 97 89C88 97 80 96 71 90C59 80 50 67 49 57C48 45 52 36 66 23C80 9 123 -12 169 -12C221 -11 288 15 342 59C403 109 431 165 431 225C431 308 366 395 238 395C212 395 165 379 127 364L153 550Z" id="g113-54"></path><glyph.data ascent="3473" descent="-2876" horiz-adv-x="480" vert-adv-y="480" xpluscharwidth="37.314"></glyph.data></g><g transform="matrix(.013,0,0,-0.013,37.314,0)"><path d="M285 378C315 398 338 416 353 432C373 451 384 474 384 503C384 579 325 635 236 635H235C182 635 136 610 108 579L65 516L85 496C110 533 150 575 205 575C258 575 300 543 300 481C300 407 232 369 141 339L147 310C163 315 188 321 211 321C268 321 338 284 338 192C338 94 288 40 217 40C160 40 119 68 93 91C85 98 77 97 69 91C60 84 47 71 46 58C44 46 48 35 62 22C75 10 116 -12 162 -12C234 -12 424 62 424 224C424 297 373 359 285 376V378Z" id="g113-52"></path><glyph.data ascent="3473" descent="-2876" horiz-adv-x="480" vert-adv-y="480" xpluscharwidth="43.554"></glyph.data></g><g transform="matrix(.013,0,0,-0.013,43.554,0)"><path d="M113 -12C146 -12 170 11 170 46C170 78 146 103 114 103S58 78 58 46C58 11 82 -12 113 -12Z" id="g113-47"></path><glyph.data ascent="3473" descent="-2876" horiz-adv-x="228" vert-adv-y="228" xpluscharwidth="46.518"></glyph.data></g><g transform="matrix(.013,0,0,-0.013,46.518,0)"><path d="M412 140C382 77 369 73 315 73H129L270 222C362 320 402 379 402 466C402 571 322 635 234 635C177 635 130 609 99 576L42 495L64 475C90 514 133 568 201 568C274 568 318 519 318 435C318 349 255 267 193 193C144 135 87 78 32 23V0H405C417 45 427 89 440 131L412 140Z" id="g113-51"></path><glyph.data ascent="3473" descent="-2876" horiz-adv-x="480" vert-adv-y="480" xpluscharwidth="52.758"></glyph.data></g></svg>, (<a href="https://static.hindawi.com/articles/ahep/volume-2017/6759267/figures/#EEq2.6">6</a>), and (<a href="https://static.hindawi.com/articles/ahep/volume-2017/6759267/figures/#EEq2.7">7</a>).

Advances in High Energy Physics

tab3

Table 3

Table 3: Starobinsky Inflation: From Non-SUSY to SUGRA Realizations 