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S. Balu

Publications and source records attributed to S. Balu.

2 recordsLinked to original sources

foraois: Fast, Flexible Extended Press-Schechter Merger Trees with a General First-Crossing Solver

We present foraois (Gaelic for Forest; FAW-reesh), an open-source Python framework for generating Monte Carlo dark matter halo merger tree histories. foraois separates the description of the linear density field, the physics of halo collapse, and the algorithmic construction of halo merger histories, allowing different cosmologies, collapse prescriptions, and tree building approaches to be combined within a common framework. The package implements two approaches to the same merger-tree problem of sampling progenitor masses in the excursion-set picture: the semi-empirical algorithm of Parkinson, Cole, & Helly (2008), which applies a fitted correction to the EPS progenitor distribution, and the numerical solution of the Markovian first-crossing equation developed by Zhang & Hui (2006), which for the default real-space top-hat window is an approximation to the correlated-walk problem. Linear matter power spectra for Cold, Warm, and Fuzzy Dark Matter (CDM, WDM, and FDM) can be supplied, while the modular collapse treatment provides an extension point for alternative barrier models. The framework also supports constrained merger histories based on the Brownian-bridge construction of Nadler et al. (2023). We run extensive validation and scaling tests, and also show an illustrative example of coupling foraois to a light-weight semi-analytical model of galaxy formation.

astro-ph.CO↗

The Impact of ionization Morphology and X-ray Heating on the Cosmological 21cm Skew Spectrum

The cosmological 21cm signal offers a potential probe of the early Universe and the first ionizing sources. Current experiments probe the spatially-dependent variance (Gaussianity) of the signal through the power spectrum (PS). The signal however is expected to be highly non-Gaussian due to the complex topology of reionization and X-ray heating. We investigate the non-Gaussianities of X-ray heating and reionization, by calculating the skew spectrum (SS) of the 21cm signal using MERAXES, which couples a semi-analytic galaxy population with semi-numerical reionization simulations. The SS is the cross-spectrum of the quadratic temperature brightness field with itself. We generate a set of seven simulations from $z = 30$ to $z = 5$, varying the halo mass threshold for hosting star-formation, the X-ray luminosity per star-formation rate, and the minimum X-ray energy escaping host galaxies. We find the SS is predominantly negative as a function of redshift, transitioning to positive towards the start of reionization, and peaking during the midpoint of reionization. We do not see a negative dip in the SS during reionization, likely due to the specifics of modelling ionization sources. We normalise the SS by the PS during reionization isolating the non-Gaussianities. We find a trough ($k\sim\,0.1\,\textrm{Mpc}^{-1}$) and peak ($k\sim\,0.4-1\,\textrm{Mpc}^{-1}$) in the normalised SS during the mid to late periods of reionization. These correlate to the ionization topology, and neutral islands in the IGM. We calculate the cosmic variance of the normalised SS, and find these features are detectable in the absence of foregrounds with the SKA_LOW.

astro-ph.CO↗