Inflation with Holographic Dark Energy

We investigate the corrections of the holographic dark energy to inflation paradigm. We study the evolution of the holographic dark energy in the inflationary universe in detail, and carry out a model-independent analysis on the holographic dark energy correction to the primordial scalar power spectrum. It turns out that the corrections generically make the spectrum redder. To be consistent with the experimental data, there must be a upper bound on the reheating temperature. We also discuss the corrections due to different choices of the infrared cutoff.Comment: 15 pages, 3 figures, v2: references added, a fast-roll discussion added. v3: typos corrected. v4: final version to appear in NP

Inflation with High Derivative Couplings

We study a class of generalized inflation models in which the inflaton is coupled to the Ricci scalar by a general $f(\phi, R)$ term. The scalar power spectrum, the spectral index, the running of the spectral index, the tensor mode spectrum and a new consistency relation of the model are calculated. We discuss in detail the issues of how to diagonize the coupled perturbation equations, how to deal with an entropy-like source, and how to determine the initial condition by quantization. By studying some explicit models, we find that rich phenomena such as a blue scalar power spectrum, a large running of the spectral index, and a blue tensor mode spectrum can be obtained.Comment: 26 pages, LaTeX; v2: refs. added; refs. correcte

The Fate of Massive Closed Strings

We calculate the semi-inclusive decay rate of an average string state with toroidal compactification in the the superstring theory. We also apply this calculation to a brane-inflation model in a warped geometry and find that the decay rate is greatly suppressed if the final strings are both massive and enhanced for massless radiation.Comment: 4 pages, to appear in the proceeding of PASCOS 2005, Gyeongju, Korea, May 30-June 4, 200

Two-scale exponential integrators with uniform accuracy for three-dimensional charged-particle dynamics under strong magnetic field

The numerical simulation of three-dimensional charged-particle dynamics (CPD) under strong magnetic field is challenging. In this paper, we introduce a new methodology to design two-scale exponential integrators for three-dimensional CPD whose magnetic field's strength is inversely proportional to a dimensionless parameter $0<\varepsilon \ll 1$. By dealing with the transformed form of three-dimensional CPD, we linearize the magnetic field and put the rest part in a nonlinear function which can be shown to be small. Based on which and the proposed two-scale exponential integrators, a class of novel integrators is formulated. The corresponding uniform accuracy over $\mathcal{O}(1/\varepsilon^{\beta})$ time interval is $\mathcal{O}(\varepsilon^{r\beta} h^r)$ for the $r$-th order integrator with the time stepsize $h$, $r=1,2,3,4$ and $0<\beta<1$. A rigorous proof of this error bound is presented and a numerical test is performed to illustrate the error behaviour of the proposed integrators