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相关论文: On the reach of perturbative methods for dark matt…

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We develop a framework for Large Scale Structure (LSS) perturbation theory, that solves the Vlasov-Poisson system of equations for the distribution function in full phase space. This approach relaxes the usual apriori assumption of…

宇宙学与河外天体物理 · 物理学 2025-06-05 Caio Nascimento , Marilena Loverde

Working within the post-Newtonian (PN) approximation to General Relativity, we use the effective field theory (EFT) framework to study the conservative dynamics of the two-body motion at fourth PN order, at fifth order in the Newton…

广义相对论与量子宇宙学 · 物理学 2017-05-17 Stefano Foffa , Pierpaolo Mastrolia , Riccardo Sturani , Christian Sturm

This work presents a formalism for deriving likelihoods of the cosmological density field directly from first principles within Perturbation Theory (PT). By assuming a perturbative expansion around the Gaussian initial density field and…

宇宙学与河外天体物理 · 物理学 2025-05-30 Rodrigo Voivodic

We perform a precision calculation of the effective field theory (EFT) conditional likelihood for large-scale structure (LSS) using the saddle-point expansion method in the presence of primordial non-Gaussianities (PNG). The precision is…

宇宙学与河外天体物理 · 物理学 2025-09-11 Ji-Yuan Ke , Yun Wang , Ping He

We study Schwinger-Keldysh effective field theories (EFTs) for systems with non-Abelian internal symmetries near thermal equilibrium. We consider two approaches that were put forward in the literature -- one using a redundant Goldstone…

高能物理 - 理论 · 物理学 2026-05-19 Eren Firat , Andrew Gomes , Filippo Nardi , Riccardo Penco , Riccardo Rattazzi

We use holographic duality to study the entanglement entropy (EE) of Conformal Field Theories (CFTs) in various spacetime dimensions $d$, in the presence of various deformations: a relevant Lorentz scalar operator with constant source, a…

高能物理 - 理论 · 物理学 2017-11-22 Nikola I. Gushterov , Andy O'Bannon , Ronnie Rodgers

The Effective Field Theory of Large-Scale Structure (EFTofLSS) provides a novel formalism that is able to accurately predict the clustering of large-scale structure (LSS) in the mildly non-linear regime. Here we provide the first…

宇宙学与河外天体物理 · 物理学 2016-10-31 Ashley Perko , Leonardo Senatore , Elise Jennings , Risa H. Wechsler

We discuss an interesting class of models, based on strongly coupled Dark Matter (DM), where sizable effects can be expected in LHC missing energy (MET) searches, compatibly with a large separation of scales. In this case, an effective…

高能物理 - 唯象学 · 物理学 2016-12-21 Sebastian Bruggisser , Francesco Riva , Alfredo Urbano

We test the regime of validity of the effective field theory (EFT) of intrinsic alignments (IA) at the one-loop level by comparing with 3D halo shape statistics in N-body simulations. This model is based on the effective field theory of…

宇宙学与河外天体物理 · 物理学 2023-03-29 Thomas Bakx , Toshiki Kurita , Nora Elisa Chisari , Zvonimir Vlah , Fabian Schmidt

The 1D flux power spectrum ($P_{\mathrm{1D}}$) of the Ly$\alpha$ forest provides an exceptionally high-resolution probe of structure formation down to small scales ($k\approx1-10~\text{$h~$Mpc$^{-1}$}$). These scales carry the imprints of…

宇宙学与河外天体物理 · 物理学 2026-04-13 N. G. Karaçaylı , M. Ivanov , R. de Belsunce , C. Ravoux , J. M. Sexton , Z. Lukić

Effective field theory (EFT) is generalized to investigate the rotational motion of triaxially deformed even-even nuclei. A Hamiltonian, called the triaxial rotor model (TRM), is obtained up to next-to-leading order (NLO) within the EFT…

核理论 · 物理学 2017-11-22 Q. B. Chen , N. Kaiser , Ulf-G. Meißner , J. Meng

We develop a new approach to study the nonlinear evolution in the large-scale structure of the Universe both in real space and in redshift space, extending the standard perturbation theory of gravitational instability. Infinite series of…

天体物理学 · 物理学 2008-11-26 Takahiko Matsubara

We reanalyze the effective field theory (EFT) approach for the scenario in which the particles that account for the dark matter (DM) in the universe are vector states that interact only through the Standard Model-like Higgs boson. These DM…

高能物理 - 唯象学 · 物理学 2023-12-22 Giorgio Arcadi , Juan Carlos Criado , Abdelhak Djouadi

In the effective field theory approach to gravity, the Lagrangian density for general relativity is supplemented by generally covariant terms of higher order in the Riemann tensor and its derivatives. At face value, these terms will result…

广义相对论与量子宇宙学 · 物理学 2024-09-25 Dražen Glavan , Shinji Mukohyama , Tom Zlosnik

This is part two in a series of papers in which we investigate an approach based on Lagrangian perturbation theory (LPT) to study the non-linear evolution of the large-scale structure distribution in the universe. Firstly, we compute the…

宇宙学与河外天体物理 · 物理学 2012-06-15 Cornelius Rampf , Yvonne Y. Y. Wong

A massive, nonrelativistic scalar field in an expanding spacetime is usually approximated by a pressureless perfect fluid, which leads to the standard conclusion that such a field can play the role of cold dark matter. In this paper, we…

宇宙学与河外天体物理 · 物理学 2020-07-14 Borna Salehian , Mohammad Hossein Namjoo , David I. Kaiser

Effective field theory (EFT) methods are applied to density functional theory (DFT) as part of a program to systematically go beyond mean-field approaches to medium and heavy nuclei. A system of fermions with short-range, natural…

核理论 · 物理学 2007-05-23 S. J. Puglia , A. Bhattacharyya , R. J. Furnstahl

We apply an orthogonalization procedure on the effective field theory of large scale structure (EFT of LSS) shapes, relevant for the angle-averaged bispectrum and non-Gaussian covariance of the matter power spectrum at one loop. Assuming…

宇宙学与河外天体物理 · 物理学 2016-11-23 Daniele Bertolini , Mikhail P. Solon

In this paper, we study the effective field theory (EFT) of dark energy for the $k$-essence model beyond linear order. Using particle-mesh $N$-body simulations that consistently solve the dark energy evolution on a grid, we find that the…

宇宙学与河外天体物理 · 物理学 2023-07-19 Farbod Hassani , Julian Adamek , Martin Kunz , Pan Shi , Peter Wittwer

Ultra-light scalar fields and their non-interacting class, the so-called fuzzy dark matter (FDM), are candidates for dark matter, introduced to solve the small-scale problems of the standard cold dark matter. In this paper, we address…

宇宙学与河外天体物理 · 物理学 2024-01-24 Hamed Manouchehri Kousha , Sina Hooshangi , Aliakbar Abolhasani