Interacting Quintessence Dark Energy Models in Lyra Manifold

<table>Squared sound speed against <svg height="8.35422pt" id="M120" style="vertical-align:-0.2130003pt" version="1.1" viewbox="-0.0498162 -8.14122 4.73688 8.35422" width="4.73688pt" xmlns="http://www.w3.org/2000/svg" xmlns:xlink="http://www.w3.org/1999/xlink"><g transform="matrix(.0135,0,0,-0.0135,0,0)"><path d="M324 430H196L233 583L223 592L145 529L120 430H54L29 396L31 388H111L56 126C33 15 54 -12 77 -12C137 -12 214 57 250 95L233 119C208 92 155 59 138 59C126 59 120 70 131 125L186 390L298 394L324 430Z" id="g113-117"></path><glyph.data ascent="3473" descent="-2876" horiz-adv-x="341" vert-adv-y="341"></glyph.data></g></svg> for the constant <svg height="9.04777pt" id="M121" style="vertical-align:-0.04981995pt" version="1.1" viewbox="-0.0498162 -8.99795 9.42853 9.04777" width="9.42853pt" xmlns="http://www.w3.org/2000/svg" xmlns:xlink="http://www.w3.org/1999/xlink"><g transform="matrix(.0135,0,0,-0.0135,0,0)"><path d="M671 0V28C608 36 593 47 562 130C495 309 432 486 368 665L336 656C270 481 202 311 134 139C98 47 84 39 20 28V0H241V28C167 38 156 47 178 115C217 236 276 383 327 530H329C375 398 437 223 484 92C499 47 489 37 424 28V0H671Z" id="g113-140"></path><glyph.data ascent="3473" descent="-2876" horiz-adv-x="686" vert-adv-y="686"></glyph.data></g></svg>. Model 1.</table>

Advances in High Energy Physics

Interacting Quintessence Dark Energy Models in Lyra Manifold

Figure 3