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相关论文: New Constraints on Warm Dark Matter from the Lyman…

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This study introduces novel constraints on the free-streaming of thermal relic warm dark matter (WDM) from Lyman-$\alpha$ forest flux power spectra. Our analysis utilises a high-resolution, high-redshift sample of quasar spectra observed…

The flux power spectrum of the high resolution Lyman-$\alpha$ forest data exhibits suppression at small scales. The origin of this suppression can be due to long-sought warm dark matter (WDM) or to thermal effects, related to the largely…

宇宙学与河外天体物理 · 物理学 2022-06-01 A. Garzilli , A. Magalich , O. Ruchayskiy , A. Boyarsky

The observed Lyman-$\alpha$ flux power spectrum (FPS) is suppressed on scales below $\sim~ 30~{\rm km~s}^{-1}$. This cutoff could be due to the high temperature, $T_0$, and pressure, $p_0$, of the absorbing gas or, alternatively, it could…

宇宙学与河外天体物理 · 物理学 2019-08-14 Antonella Garzilli , Andrii Magalich , Tom Theuns , Carlos S. Frenk , Christoph Weniger , Oleg Ruchayskiy , Alexey Boyarsky

High resolution N-body simulations of cold dark matter (CDM) models predict that galaxies and clusters have cuspy halos with excessive substructure. Observations reveal smooth halos with central density cores. One possible resolution of…

天体物理学 · 物理学 2015-09-23 Vijay K. Narayanan , David N. Spergel , Romeel Davé , Chung-Pei Ma

We present updated constraints on the free-streaming of warm dark matter (WDM) particles derived from an analysis of the Lya flux power spectrum measured from high-resolution spectra of 25 z > 4 quasars obtained with the Keck High…

宇宙学与河外天体物理 · 物理学 2015-06-16 M. Viel , G. D. Becker , J. S. Bolton , M. G. Haehnelt

This study sets new constraints on Cold+Warm Dark Matter (CWDM) models by leveraging the small-scale suppression of structure formation imprinted in the Lyman-$\alpha$ forest. Using the Sherwood-Relics suite, we extract high-fidelity flux…

宇宙学与河外天体物理 · 物理学 2025-08-29 Olga Garcia-Gallego , Vid Iršič , Martin G. Haehnelt , Matteo Viel , James S. Bolton

We present new measurements of the free-streaming of warm dark matter (WDM) from Lyman-$\alpha$ flux-power spectra. We use data from the medium resolution, intermediate redshift XQ-100 sample observed with the X-shooter spectrograph ($z=3 -…

In this paper we present an efficient method for constraining both thermal and non-thermal Dark Matter (DM) scenarios with the Lyman-$\alpha$ forest, based on a simple and flexible parametrisation capable to reproduce the small scale…

宇宙学与河外天体物理 · 物理学 2018-11-07 Riccardo Murgia , Vid Iršič , Matteo Viel

We present an analysis of high-resolution N-body simulations of decaying dark matter cosmologies focusing on the statistical properties of the transmitted Lyman-alpha forest flux in the high-redshift intergalactic medium. In this type of…

宇宙学与河外天体物理 · 物理学 2015-06-17 Mei-Yu Wang , Rupert A. C. Croft , Annika H. G. Peter , Andrew R. Zentner , Chris W. Purcell

We investigate Lyman-alpha forest flux statistics in mixed fuzzy dark matter (FDM) and cold dark matter (CDM) cosmologies using the Fluctuating Gunn-Peterson Approximation (FGPA) applied to hybrid Schr\"odinger-Poisson and N-body…

宇宙学与河外天体物理 · 物理学 2026-04-08 Yourong Frank Wang

The Lyman-$\alpha$ forest is a valuable probe of dark matter models featuring a scale-dependent suppression of the power spectrum as compared to $\Lambda$CDM. In this work, we present a new estimator of the Lyman-$\alpha$ flux power…

宇宙学与河外天体物理 · 物理学 2018-09-19 Mathias Garny , Thomas Konstandin , Laura Sagunski , Sean Tulin

If a significant fraction of the dark matter in the Universe is made of an ultra-light scalar field, named fuzzy dark matter (FDM) with a mass $m_a$ of the order of $10^{-22}-10^{-21}$ eV, then its de Broglie wavelength is large enough to…

宇宙学与河外天体物理 · 物理学 2017-08-22 Eric Armengaud , Nathalie Palanque-Delabrouille , Christophe Yèche , David J. E. Marsh , Julien Baur

We present constraints on the mass of warm dark matter (WDM) particles derived from the Lyman-alpha flux power spectrum of 55 high- resolution HIRES spectra at 2.0 < z < 6.4. From the HIRES spectra, we obtain a lower limit of mwdm > 1.2 keV…

天体物理学 · 物理学 2008-11-26 M. Viel , G. D. Becker , J. S. Bolton , M. G. Haehnelt , M. Rauch , W. L. W. Sargent

We present constraints on the masses of extremely light bosons dubbed fuzzy dark matter from Lyman-$\alpha$ forest data. Extremely light bosons with a De Broglie wavelength of $\sim 1$ kpc have been suggested as dark matter candidates that…

宇宙学与河外天体物理 · 物理学 2017-08-01 Vid Iršič , Matteo Viel , Martin G. Haehnelt , James S. Bolton , George D. Becker

We review the current state of the theory of large scale structure in a warm dark matter (WDM) cosmological model. In particular, we focus on the non-linear modelling of the matter power spectrum and on the mass function of dark matter…

宇宙学与河外天体物理 · 物理学 2014-02-18 Katarina Markovič , Matteo Viel

Decaying Cold Dark Matter (DCDM) is a model that is currently under investigation regarding primarily the $S_8$ tension between cosmic microwave background (CMB) and certain large-scale structure measurements. The decay into one massive and…

宇宙学与河外天体物理 · 物理学 2022-10-13 Lea Fuß , Mathias Garny

The 3D distribution of matter at small scales encodes valuable information about the nature of dark matter and other fundamental physics. A prominent probe of such scales outside galaxies is the Lyman-alpha forest, which studies absorption…

宇宙学与河外天体物理 · 物理学 2025-05-21 Ivan Ridkokasha , Andres Aramburo-Garcia , Kyrylo Bondarenko , Anastasia Sokolenko , Matthieu Schaller , Alexey Boyarsky

The ultralight dark photon is a well-motivated, hypothetical dark matter candidate. In a dilute plasma, they can resonantly convert into photons, and heat up the intergalactic medium between galaxies. In this work, we explore the dark…

宇宙学与河外天体物理 · 物理学 2025-04-04 Andrea Trost , James S. Bolton , Andrea Caputo , Hongwan Liu , Stefano Cristiani , Matteo Viel

With recent Lyman-alpha forest data from BOSS and XQ-100, some studies suggested that the lower mass limit on the fuzzy dark matter (FDM) particles is lifted up to $10^{-21}\,\mathrm{eV}$. However, such a limit was obtained by $\Lambda$CDM…

宇宙学与河外天体物理 · 物理学 2018-08-14 Jiajun Zhang , Jui-Lin Kuo , Hantao Liu , Yue-Lin Sming Tsai , Kingman Cheung , Ming-Chung Chu

We use LUQAS, a sample of 27 high resolution high signal-to-noise UVES quasar (QSO) spectra (Kim et al. 2004), and the Croft et al. (2002) sample together with a set of high resolution large box size hydro-dynamical simulations run with the…

天体物理学 · 物理学 2009-11-11 Matteo Viel
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