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We take an Effective Field Theory (EFT) approach to unifying existing proposals for the origin of cosmic acceleration and its connection to cosmological observations. Building on earlier work where EFT methods were used with observations to…

宇宙学与河外天体物理 · 物理学 2013-09-24 Jolyon K. Bloomfield , Éanna É. Flanagan , Minjoon Park , Scott Watson

We formulate an effective field theory (EFT) of coupled dark energy (DE) and dark matter (DM) interacting through energy and momentum transfers. In the DE sector, we exploit the EFT of vector-tensor theories with the presence of a preferred…

宇宙学与河外天体物理 · 物理学 2026-02-24 Katsuki Aoki , Jose Beltrán Jiménez , Masroor C. Pookkillath , Shinji Tsujikawa

The Effective Field Theory of Large Scale Structure (EFTofLSS) has found tremendous success as a perturbative framework for the evolution of large scale structure, and it is now routinely used to compare theoretical predictions against…

宇宙学与河外天体物理 · 物理学 2025-02-18 Caio Nascimento , Drew Jamieson , Matthew McQuinn , Marilena Loverde

In this paper we present an extension to the $\texttt{matryoshka}$ suite of neural-network-based emulators. The new editions have been developed to accelerate EFTofLSS analyses of galaxy power spectrum multipoles in redshift space. They are…

宇宙学与河外天体物理 · 物理学 2022-11-30 Jamie Donald-McCann , Kazuya Koyama , Florian Beutler

We present a new model for the redshift-space power spectrum of galaxies and demonstrate its accuracy in modeling the monopole, quadrupole, and hexadecapole of the galaxy density field down to scales of $k = 0.4 \ h\mathrm{Mpc}^{-1}$. The…

宇宙学与河外天体物理 · 物理学 2017-10-18 Nick Hand , Uros Seljak , Florian Beutler , Zvonimir Vlah

Effective Field Theories (EFTs) constructed as derivative expansions in powers of momentum, in the spirit of Chiral Perturbation Theory (ChPT), are a controllable approximation to strong dynamics as long as the energy of the interacting…

高能物理 - 唯象学 · 物理学 2021-08-11 Alexandre Salas-Bernárdez , Felipe J. Llanes-Estrada , Juan Escudero-Pedrosa , Jose Antonio Oller

We explore the Lagrangian perturbation theory (LPT) at 1-loop order with Gaussian initial conditions. We present an expansion method to approximately compute the power spectrum in LPT. Our approximate solution has good convergence in the…

宇宙学与河外天体物理 · 物理学 2015-06-17 Naonori S. Sugiyama

We generalize previously derived analytic results for the one-loop power spectrum (PS) in scale-free models (with linear PS $P(k) \propto k^n$) to a broader class of such models in which part of the matterlike component driving the Einstein…

宇宙学与河外天体物理 · 物理学 2023-07-31 Azrul Pohan , Michael Joyce , David Benhaiem , Francesco Sylos Labini

We present the effective-field theory (EFT)-based cosmological full-shape analysis of the anisotropic power spectrum of eBOSS quasars at the effective redshift $z_{\rm eff}=1.48$. We perform extensive tests of our pipeline on simulations,…

宇宙学与河外天体物理 · 物理学 2023-02-22 Anton Chudaykin , Mikhail M. Ivanov

We present an efficient and accurate pipeline for the analysis of the redshift-space galaxy bispectrum multipoles at one-loop order in effective field theory (EFT). We provide a systematic theory derivation based on power counting, which…

宇宙学与河外天体物理 · 物理学 2025-12-05 Thomas Bakx , Mikhail M. Ivanov , Oliver H. E. Philcox , Zvonimir Vlah

The anisotropy of clustering in redshift space provides a direct measure of the growth rate of large scale structure in the Universe. Future galaxy redshift surveys will make high precision measurements of these distortions, and will…

宇宙学与河外天体物理 · 物理学 2010-10-28 Elise Jennings , Carlton M. Baugh , Silvia Pascoli

We derive an effective field theory (EFT) for cosmological Lyman alpha forest fluctuations valid for the power spectrum at the one-loop order. The ``bottom-up'' EFT expansion at the level of the transmitted flux is identical to the…

宇宙学与河外天体物理 · 物理学 2024-01-04 Mikhail M. Ivanov

Constraints on gravity and cosmology will greatly benefit from performing joint clustering and weak lensing analyses on large-scale structure data sets. Utilising non-linear information coming from small physical scales can greatly enhance…

宇宙学与河外天体物理 · 物理学 2020-08-17 Benjamin Bose , Hans A. Winther , Alkistis Pourtsidou , Santiago Casas , Lucas Lombriser , Qianli Xia , Matteo Cataneo

We apply the Wiener Hermite (WH) expansion to the non-linear evolution of Large-Scale Structure, and obtain an approximate expression for the matter power spectrum in full order of the expansion. This method allows us to expand any random…

宇宙学与河外天体物理 · 物理学 2015-06-11 Naonori S. Sugiyama , Toshifumi Futamase

We present the first systematic derivation of the one-loop correction to the large scale matter power spectrum in a mixed cold+hot dark matter cosmology with subdominant massive neutrino hot dark matter. Starting with the equations of…

天体物理学 · 物理学 2009-11-19 Yvonne Y. Y. Wong

Using a full implementation of resummed perturbation theory (PT) from a multi-point propagator expansion, we put forward new theoretical predictions for the two-point statistics of matter fluctuations in redshift space. The predictions…

宇宙学与河外天体物理 · 物理学 2013-04-10 Atsushi Taruya , Takahiro Nishimichi , Francis Bernardeau

Over the next decade, cosmological measurements of the large-scale structure of the Universe will be sensitive to the combined effects of dynamical dark energy and massive neutrinos. The matter power spectrum is a key repository of this…

宇宙学与河外天体物理 · 物理学 2014-05-21 Amol Upadhye , Rahul Biswas , Adrian Pope , Katrin Heitmann , Salman Habib , Hal Finkel , Nicholas Frontiere

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

Recently, we find that the correction for the EdS assumption on the one-loop matter power spectrum for general dark energy models using the standard perturbation theory is not negligible \cite{LPB}. Thus, we investigate the same problem by…

宇宙学与河外天体物理 · 物理学 2014-11-07 Seokcheon Lee

We extend field-level inference to jointly constrain the cosmological parameters $\{A,\omega_{\rm cdm},H_0\}$, in both real and redshift space. Our analyses are based on mock data generated using a perturbative forward model, with noise…

宇宙学与河外天体物理 · 物理学 2025-09-25 Kazuyuki Akitsu , Marko Simonović , Shi-Fan Chen , Giovanni Cabass , Matias Zaldarriaga