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相关论文: Lattice Refining Loop Quantum Cosmology and Inflat…

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In the context of loop quantum cosmology, we consider an inflationary era driven by a canonical scalar field and occurring in the semiclassical regime, where spacetime is a continuum but quantum gravitational effects are important. The…

广义相对论与量子宇宙学 · 物理学 2009-11-11 Gianluca Calcagni , Marina Cortes

Inflationary models of the early universe provide a natural mechanism for the formation of large scale structure. This success brings to forefront the question of naturalness: Does a sufficiently long slow roll inflation occur generically…

广义相对论与量子宇宙学 · 物理学 2015-05-27 Abhay Ashtekar , David Sloan

We study numerically the decay of the inflaton by solving the full non-linear equations of motion on the lattice. We confirm that parametric resonance is effective in transferring energy from the inflaton to a scalar field as long as the…

高能物理 - 唯象学 · 物理学 2009-10-30 Tomislav Prokopec , Thomas G. Roos

This paper discusses the problem of inflation in the context of Friedmann-Robertson-Walker Cosmology. We show how, after a simple change of variables, one can quantize the problem in a way which parallels the classical discussion. The…

高能物理 - 理论 · 物理学 2007-05-23 Marvin Weinstein , Ratin Akhoury

The first aim of this lecture is to highlight two areas of recent progress in inflationary cosmology, namely reheating and the quantum theory of cosmological perturbations. The second aim is to discuss important conceptual problems for the…

高能物理 - 唯象学 · 物理学 2007-05-23 Robert H. Brandenberger

In the context of group field theory condensate cosmology, we clarify the extraction of cosmological variables from the microscopic quantum gravity degrees of freedom. We show that an important implication of the second quantized formalism…

广义相对论与量子宇宙学 · 物理学 2014-12-03 Steffen Gielen , Daniele Oriti

We use a lattice simulation to study a model of axion inflation where the inflaton is coupled to a U(1) gauge field through Chern-Simons interaction. These kinds of models have already been studied with a lattice simulation in the context…

宇宙学与河外天体物理 · 物理学 2022-06-28 Angelo Caravano , Eiichiro Komatsu , Kaloian D. Lozanov , Jochen Weller

We present the detailed analyses of five-dimensional loop quantum Kaluza-Klein cosmology based on the symmetric reduction of the connection formulation of the full theory. The previous results in a particular scenario are extended to more…

广义相对论与量子宇宙学 · 物理学 2026-05-28 Shengzhi Li , Yongge Ma , Faqiang Yuan , Xiangdong Zhang

Inflation models can have an early phase of inflation where the evolution of the inflaton is driven by quantum fluctuations before entering the phase driven by the slope of the scalar field potential. For a Coleman-Weinberg potential this…

宇宙学与河外天体物理 · 物理学 2013-03-06 Arjun Berera , Raghavan Rangarajan

The standard model of cosmology assumes a homogeneous and isotropic universe that undergoes a period of exponential expansion very early on, named inflation. This stretches quantum fluctuations from the onset of inflation to cosmological…

广义相对论与量子宇宙学 · 物理学 2024-10-22 Rita B. Neves

We study the scalar modes of linear perturbations in loop quantum cosmology. This is done on a lattice where each cell is taken to be homogeneous and isotropic and can be quantized via standard homogeneous loop quantum cosmology techniques.…

广义相对论与量子宇宙学 · 物理学 2015-06-05 Edward Wilson-Ewing

Inflation in the early Universe is one of the most promising probes of gravity in the high-energy regime. However, observable scales give access to a limited window in the inflationary dynamics. In this essay, we argue that quantum…

高能物理 - 理论 · 物理学 2017-11-22 Robert J. Hardwick , Vincent Vennin , David Wands

We investigate the corrections to the inflationary cosmological dynamics due to a $R^2$ term in the Palatini formulation which may arise as quantum corrections to the effective Lagrangian in early universe. We found that the standard…

广义相对论与量子宇宙学 · 物理学 2009-11-10 Xin-He Meng , Peng Wang

A special class of conformal gravity theories is proposed to solve the long standing problem of the fine-tuned cosmological constant. In the proposed model time evolution of the inflaton field leaves behind a nearly vanishing, but finite…

高能物理 - 唯象学 · 物理学 2022-04-25 M. Yoshimura

Based on the conventional metric tensor and driven by a nearly constant energy density, cosmic inflation, characterized by a remarkably accelerated expansion, was proposed as an early epoch in the Universe. The energy density is typically…

广义相对论与量子宇宙学 · 物理学 2026-05-05 Swapnil K. Singh , Saleh O. Allehabi , Azzah A. Alshehri , Mahmoud Nasar , Abdel Nasser Tawfik

The relaxion scenario presents an intriguing extension of the standard model in which the particle introduced to solve to the strong CP problem, the axion, also achieves the dynamical relaxation of the Higgs boson mass term. In this work we…

高能物理 - 唯象学 · 物理学 2016-09-09 Stefano Di Chiara , Kristjan Kannike , Luca Marzola , Antonio Racioppi , Martti Raidal , Christian Spethmann

Loop quantum cosmology (LQC) provides promising resolutions to the trans-Planckian issue and initial singularity arising in the inflationary models of general relativity. In general, due to different quantization approaches, LQC involves…

广义相对论与量子宇宙学 · 物理学 2015-12-10 Tao Zhu , Anzhong Wang , Gerald Cleaver , Klaus Kirsten , Qin Sheng , Qiang Wu

A semiclassical description of quantum systems is applied to probe the dynamics of the cosmological model of an inflationary universe with quadratic inflaton potential, described in a quantum framework of geometrodynamics. The systematic…

广义相对论与量子宇宙学 · 物理学 2022-10-27 David Brizuela , Tomasz Pawlowski

We reconsider the fine-tuning problem of scalar-driven inflation arising from the need to couple the inflaton to ordinary matter in order to make reheating efficient. Quantum fluctuations of this matter induce Coleman-Weinberg corrections…

广义相对论与量子宇宙学 · 物理学 2019-11-13 S. P. Miao , S. Park , R. P. Woodard

We present a lattice formulation of an interaction ${\phi\over\Lambda} F\tilde F$ between an axion and some $U(1)$ gauge sector with the following properties: it reproduces the continuum theory up to $\mathcal{O}(dx_\mu^2)$ corrections, it…

宇宙学与河外天体物理 · 物理学 2019-06-12 Jose Roberto Canivete Cuissa , Daniel G. Figueroa