The DSpace digital repository system captures, stores, indexes, preserves, and distributes digital research material. http://dspace-roma3.caspur.it:80 2013-05-18T21:18:42Z 2013-05-18T21:18:42Z Viel, Matteo Branchini, Enzo Dolag, Klaus Grossi, Margherita Matarrese, Sabino Moscardini, Lauro http://hdl.handle.net/2307/225 2011-12-22T13:34:55Z 2008-12-31T23:00:00Z

<Title>Primordial non-Gaussianities in the intergalactic medium</Title> <Authors>Viel, Matteo; Branchini, Enzo; Dolag, Klaus; Grossi, Margherita; Matarrese, Sabino; Moscardini, Lauro</Authors> <Issue Date>2009</Issue Date> <Is part of>Monthly notices of the Royal Astronomical Society</Is part of> <Volume>393</Volume> <Pages>774-782</Pages> <Abstract>We present results from the first high-resolution hydrodynamical simulations of non-Gaussian cosmological models. We focus on the statistical properties of the transmitted Lyman-alpha flux in the high-redshift intergalactic medium. Imprints of non-Gaussianity are present and are larger at high redshifts. Differences larger than 20 per cent at z > 3 in the flux probability distribution function for high-transmissivity regions (voids) are expected for values of the non-linearity parameter f(NL) = +/- 100 when compared to a standard Lambda cold dark matter cosmology with f(NL) = 0. We also investigate the one-dimensional flux bispectrum: at the largest scales(corresponding to tens of Mpc), we expect deviations in the flux bispectrum up to 20 per cent at z similar to 4 (for f(NL) = +/- 100),significantly larger than deviations of similar to 3 per cent in the flux power spectrum. We briefly discuss possible systematic errors that can contaminate the signal. Although challenging, a detection of non-Gaussianities in the interesting regime of scales and redshifts probed by the Lyman-alpha forest could be possible with future data sets.</Abstract>

2008-12-31T23:00:00Z