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相关论文: On the effect of the ionising background on the Ly…

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The \lya forest at high redshifts is a powerful probe of reionization. Modeling and observing this imprint comes with significant technical challenges: inhomogeneous reionization must be taken into account while simultaneously being able to…

宇宙学与河外天体物理 · 物理学 2019-05-21 Paulo Montero-Camacho , Christopher M. Hirata , Paul Martini , Klaus Honscheid

Murphy et al. (2003a, MNRAS, 345, 609) claim to find evidence of cosmological variations of the fine structure constant $\alpha$ in the spectra of intervening QSO absorption line systems. We find that this result is affected by systematic…

天体物理学 · 物理学 2016-08-30 Rino Bandiera , Edvige Corbelli

We present predictions of the correlation between the Lyman-alpha forest absorption in quasar spectra and the mass within \sim 5 Mpc/h (comoving) of the line of sight, using fully hydrodynamic and hydro-PM numerical simulations of the cold…

天体物理学 · 物理学 2009-11-07 Patrick McDonald , Jordi Miralda-Escudé , Renyue Cen

We investigate the relationship between the Lyman-alpha (Lya) forest transmission in the intergalactic medium (IGM) and the environmental density of galaxies, focusing on its implications for the measurement of ionizing radiation escape…

We investigate possible systematic errors in the recent measurement of the matter power spectrum from the Lyman-alpha forest by Croft et al. (2001). We find that for a large set of prior cosmological models the Croft et al. result holds…

天体物理学 · 物理学 2009-11-07 Nickolay Y. Gnedin , Andrew J. S. Hamilton

We investigate the possibility of constraining primordial non-Gaussianity using the 3D bispectrum of Ly-alpha forest. The strength of the quadratic non-Gaussian correction to an otherwise Gaussian primordial gravitational field is assumed…

宇宙学与河外天体物理 · 物理学 2012-09-19 Dhiraj Kumar Hazra , Tapomoy Guha Sarkar

Reionization leads to large spatial fluctuations in the intergalactic temperature that can persist well after its completion. We study the imprints of such fluctuations on the $z\sim5$ Ly$\alpha$ forest flux power spectrum using a set of…

宇宙学与河外天体物理 · 物理学 2019-10-07 Xiaohan Wu , Matthew McQuinn , Rahul Kannan , Anson D'Aloisio , Simeon Bird , Federico Marinacci , Romeel Davé , Lars Hernquist

The low density hydrogen and helium in the IGM probed by QSO absorption lines is sensitive to the amplitude and spectral shape of the metagalactic UV background. We use realistic HI and HeII Ly-alpha forest spectra, constructed from…

天体物理学 · 物理学 2009-11-13 James S. Bolton , Martin G. Haehnelt , Matteo Viel , Robert F. Carswell

We investigate the dependence of QSO Lyman-alpha absorption features on the temperature of the absorbing gas and on the amplitude of the underlying dark matter fluctuations. We use high-resolution hydrodynamic simulations in cold dark…

天体物理学 · 物理学 2009-10-31 Tom Theuns , Joop Schaye , Martin Haehnelt

The peculiar velocities of galaxies distort the pattern of galaxy clustering in redshift space, making the redshift space power spectrum anisotropic. In the linear regime, the strength of this distortion depends only on the ratio $\beta…

天体物理学 · 物理学 2015-06-24 Shaun Cole , Karl B. Fisher , David H. Weinberg

We quantify the contribution of Ly$\alpha$ fluorescence to observed spatially extended Ly$\alpha$ halos around Ly$\alpha$ emitters (LAE) at redshift ${\rm z=3.1}$. The key physical quantities that describe the fluorescent signal include…

星系天体物理 · 物理学 2016-05-25 Lluís Mas-Ribas , Mark Dijkstra

The post-reionization thermal state of the intergalactic medium is characterized by a power-law relationship between temperature and density, with a slope determined by the parameter $\gamma$. We describe a new method to measure $\gamma$…

宇宙学与河外天体物理 · 物理学 2015-12-16 Elisa Boera , Michael T. Murphy , George D. Becker , James S. Bolton

We use the Sherwood-Relics suite of hybrid hydrodynamical and radiative transfer simulations to model the effect of inhomogeneous reionisation on the 1D power spectrum of the \Lya forest transmitted flux at redshifts $4.2\leq z \leq 5$.…

The observed scatter in intergalactic Lyman-$\alpha$ opacity at $z \lesssim 6$ requires large-scale fluctuations in the neutral fraction of the intergalactic medium (IGM) after the expected end of reionization. Post-reionization models that…

宇宙学与河外天体物理 · 物理学 2018-08-22 George D. Becker , Frederick B. Davies , Steven R. Furlanetto , Matthew A. Malkan , Elisa Boera , Craig Douglass

Using a suite of hydrodynamical simulations with cold dark matter, baryons, and neutrinos, we present a detailed study of the effect of massive neutrinos on the 1-D and 3-D flux power spectra of the Lyman-$\alpha$ (Ly$\alpha$) forest. The…

Absorption between the rest-frame wavelengths of 973 and 1026 Angstroms in quasar spectra arises from two sources (apart from occasional metals): one is due to Lyman-alpha (Lya) absorption by materials at a low redshift, and the other from…

天体物理学 · 物理学 2009-11-07 Mark Dijkstra , Adam Lidz , Lam Hui

The currently observing Dark Energy Spectroscopic Instrument (DESI) places sub-percent constraints on the Baryon Acoustic Oscillations (BAO) scaling parameters from the Lyman-$\alpha$ (Ly-$\alpha$) forest. However, no systematic error…

宇宙学与河外天体物理 · 物理学 2025-03-18 Boryana Hadzhiyska , Roger de Belsunce , Andrei Cuceu , Julien Guy , Mikhail M. Ivanov , Henri Coquinot , Andreu Font-Ribera

It has been recently shown that the astrophysics of reionization can be extracted from the Ly$\alpha$ forest power spectrum by marginalizing the memory of reionization over cosmological information. This impact of cosmic reionization on the…

宇宙学与河外天体物理 · 物理学 2023-03-07 Paulo Montero-Camacho , Yuchen Liu , Yi Mao

We investigate the cross-correlation signal between 21cm intensity mapping maps and the Lyman-alpha forest in the fully non-linear regime using state-of-the-art hydrodynamic simulations. The cross-correlation signal between these fields can…

宇宙学与河外天体物理 · 物理学 2017-04-06 Isabella P. Carucci , Francisco Villaescusa-Navarro , Matteo Viel

The large opacity fluctuations in the $z > 5.5$ Ly$\alpha$ forest may indicate inhomogeneous progress of reionization. To explain the observed large scatter of the effective Ly$\alpha$ optical depth ($\tau_{\rm eff}$) of the intergalactic…