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In single-field inflationary models with a low sound speed, the orthogonal shape of the primordial bispectrum arises due to partial cancellations between equilateral-type shapes. This fact allows for a speed of sound c_s as low as about…

宇宙学与河外天体物理 · 物理学 2015-06-15 Sebastien Renaux-Petel

Recent measurements of the $4$-point correlation functions (4PCF) from spectroscopic surveys provide evidence for parity-violations in the large-scale structure of the Universe. If physical in origin, this could point to exotic physics…

宇宙学与河外天体物理 · 物理学 2023-12-18 Peter L. Taylor , Matthew Craigie , Yuan-Sen Ting

Cosmological correlation functions of inflaton and graviton perturbations are the fundamental observables of early universe cosmology and remain a primary target for observations. In this work, we ask the following question: are these…

高能物理 - 理论 · 物理学 2026-04-15 David Stefanyszyn , Xi Tong , Yuhang Zhu

We study the reconstruction of the cosmic rotation power spectrum produced by parity-violating physics, with an eye to ongoing and near future cosmic microwave background (CMB) experiments such as BICEP Array, CMBS4, LiteBIRD and Simons…

宇宙学与河外天体物理 · 物理学 2019-11-27 Toshiya Namikawa

We investigate the cosmic microwave background (CMB) bispectra of the intensity (temperature) and polarization modes induced by the graviton non-Gaussianities, which arise from the parity-conserving and parity-violating Weyl cubic terms…

宇宙学与河外天体物理 · 物理学 2012-02-14 Maresuke Shiraishi , Daisuke Nitta , Shuichiro Yokoyama

We compute the 3-point correlation function for a general model of inflation driven by a single, minimally coupled scalar field. Our approach is based on the numerical evaluation of both the perturbation equations and the integrals which…

天体物理学 · 物理学 2010-10-27 Xingang Chen , Richard Easther , Eugene A. Lim

A no-go theorem for parity-violation in even $D$-dimensional spacetimes invariant under $ISO(d)$ and dilatations (as well as the implications for odd $D$) is derived. For the case of real massless scalar and gravitons (as well as any…

高能物理 - 理论 · 物理学 2025-08-06 Ayngaran Thavanesan

Pseudoscalar or pseudovector cosmic fields, that serve as a source of parity ($\mathcal{P}$) violation, are invoked in different models for cold dark matter or in the standard model extension that allows for Lorentz invariance violation. A…

化学物理 · 物理学 2020-09-23 Konstantin Gaul , Mikhail G. Kozlov , Timur A. Isaev , Robert Berger

Non-Gaussianities of the primordial density perturbations have emerged as a very powerful possible signal to test the dynamics that drove the period of inflation. While in general the most sensitive observable is the three-point function in…

高能物理 - 理论 · 物理学 2011-01-17 Leonardo Senatore , Matias Zaldarriaga

During single clock inflation, hidden fields (i.e. fields coupled to the inflaton only gravitationally) in their adiabatic vacua can ordinarily only affect observables through virtual effects. After renormalizing background quantities…

广义相对论与量子宇宙学 · 物理学 2019-01-30 Adrian del Rio , Ruth Durrer , Subodh P. Patil

We derive constraints on three-point functions involving the stress tensor, $T$, and a conserved $U(1)$ current, $j$, in 2+1 dimensional conformal field theories that violate parity, using conformal collider bounds introduced by Hofman and…

高能物理 - 理论 · 物理学 2017-09-22 Subham Dutta Chowdhury , Justin R. David , Shiroman Prakash

Some recent observations of the cosmic microwave background (CMB) anisotropies and the large-scale structure of the Universe imply cosmic parity violation. Among possible parity-violating sources, helical primordial magnetic fields (PMFs)…

宇宙学与河外天体物理 · 物理学 2025-06-12 Kaito Yura , Shohei Saga , Maresuke Shiraishi , Shuichiro Yokoyama

In a variety of inflation models the motion of the inflaton may trigger the production of some non-inflaton particles during inflation, for example via parametric resonance or a phase transition. Particle production during inflation leads…

宇宙学与河外天体物理 · 物理学 2010-01-07 Neil Barnaby , Zhiqi Huang

We generalize the Effective Field Theory of Inflation to include additional light scalar degrees of freedom that are in their vacuum at the time the modes of interest are crossing the horizon. In order to make the scalars light in a natural…

高能物理 - 理论 · 物理学 2015-05-19 Leonardo Senatore , Matias Zaldarriaga

If cosmic inflation suffered tiny time-dependent deviations from the slow-roll regime, these would induce the existence of small scale-dependent features imprinted in the primordial spectra, with their shapes and sizes revealing information…

宇宙学与河外天体物理 · 物理学 2016-09-21 Sander Mooij , Gonzalo A. Palma , Grigoris Panotopoulos , Alex Soto

We describe models of single-field inflation with small and sharp step features in the potential (and sound speed) of the inflaton field, in the context of the Effective Field Theory of Inflation. This approach allows us to study the…

宇宙学与河外天体物理 · 物理学 2015-06-16 Nicola Bartolo , Dario Cannone , Sabino Matarrese

We examine the origin of the cosmological collider signal using the framework of open effective field theories. Focusing on the single exchange of a massive scalar field, we demonstrate that the trispectrum splits cleanly into its local and…

高能物理 - 理论 · 物理学 2025-12-10 Thomas Colas , Zhehan Qin , Xi Tong

In the present thesis, using an effective field theory point of view, we explore theories of single-field inflation where higher derivative operators become relevant, affecting in a novel way the dynamics and therefore the observations. For…

高能物理 - 理论 · 物理学 2016-12-06 Luca Santoni

In direct analogy to the 4-body decay of a heavy scalar particle, the 4-point correlation function of primordial fluctuations carries P and CP information. The CP violation appears as a P-odd angular dependence in the imaginary part of the…

高能物理 - 唯象学 · 物理学 2020-05-20 Tao Liu , Xi Tong , Yi Wang , Zhong-Zhi Xianyu

The Cosmic Microwave Background can provide information regarding physics of the very early universe, more specifically, of the matter-radiation distribution of the inflationary era. Starting from the effective field theory of inflation, we…

高能物理 - 理论 · 物理学 2015-09-02 Anindya Banerjee , Himanshu Khanchandani