Trapped quintessential inflation
Trapped quintessential inflation
复制标题
典型的通胀受困
DOI：
10.1016/j.physletb.2006.09.045
复制
发表时间：
2006
影响因子：
4.4
通讯作者：
K. Dimopoulos
中科院分区：
文献类型：
--
作者：
J. C. B. Sánchez;K. Dimopoulos
使用弦模作为膨胀-本质场来研究本质膨胀。模量在其标量势的陡峭部分开始演变，这是由于非微扰效应（例如，高吉诺凝聚）。假设模场穿过场空间中的增强对称点（ESP）。ESP处的颗粒产生暂时捕获模量，导致短暂的膨胀。由于势的平坦性，更多的膨胀随之而来，因为ESP在标量势中产生极值（最大值或最小值）或平坦的拐点。最后，潜在的风险再次变得陡峭，通货膨胀终止。在重新加热后，由于宇宙学摩擦，模量冻结在一个大的值，这样它的标量势就被额外维度的通量或其他效应所支配。模量保持冻结，直到现在，当它可以成为精髓，并解释暗能量所必需的解释观察到的加速膨胀。
Quintessential inflation is studied using a string modulus as the inflaton–quintessence field. The modulus begins its evolution at the steep part of its scalar potential, which is due to non-perturbative effects (e.g. gaugino condensation). It is assumed that the modulus crosses an enhanced symmetry point (ESP) in field space. Particle production at the ESP temporarily traps the modulus resulting in a brief period of inflation. More inflation follows, due to the flatness of the potential, since the ESP generates either an extremum (maximum or minimum) or a flat inflection point in the scalar potential. Eventually, the potential becomes steep again and inflation is terminated. After reheating the modulus freezes due to cosmological friction at a large value, such that its scalar potential is dominated by contributions due to fluxes in the extra dimensions or other effects. The modulus remains frozen until the present, when it can become quintessence and account for the dark energy necessary to explain the observed accelerated expansion.
规范介导的 SUSY 断裂中的 MSSM 曲线
DOI：
--
发表时间：
2004
期刊：
Physics Letters B 578
影响因子：
--
作者：
S.Kasuya;M.Kawasaki;F.Takahashi
通讯作者：
F.Takahashi
影响因子：
8.6
作者：
I. Zlatev;Limin Wang;Paul J. Steinhardt University of Pennsylvania;P. University
通讯作者：
I. Zlatev;Limin Wang;Paul J. Steinhardt University of Pennsylvania;P. University