265 citations · 5.1k across the 125 of their papers we have counts for
10 papers · 1 filter
nIFTy Galaxy Cluster simulations VI: The dynamical imprint of substructure on gaseous cluster outskirts
C. Power, P. J. Elahi, C. Welker +11
Galaxy cluster outskirts mark the transition region from the mildly non-linear cosmic web to the highly non-linear, virialised, cluster interior. It is in this transition region th…
Large Lyman-alpha opacity fluctuations and low CMB tau in models of late reionization with large islands of neutral hydrogen extending to z<5.5
Girish Kulkarni, Laura C. Keating, Martin G. Haehnelt +4
High-redshift QSO spectra show large spatial fluctuations in the Ly-alpha opacity of the intergalactic medium on surprisingly large scales at z>~5.5. We present a radiative transfe…
Missing Gamma-ray Halos and the Need for New Physics in the Gamma-ray Sky
Avery E. Broderick, Paul Tiede, Philip Chang +5
An intergalactic magnetic field stronger than ~G would explain the lack of a bright, extended degree-scale, GeV-energy inverse Compton component in the gamma-ray s…
The modified gravity lightcone simulation project I: Statistics of matter and halo distributions
Christian Arnold, Pablo Fosalba, Volker Springel +2
We introduce a set of four very high resolution cosmological simulations for exploring -gravity, with particles in and $1536\,h^{-1}\textrm…
Enhancing AGN efficiency and cool-core formation with anisotropic thermal conduction
David J. Barnes, Rahul Kannan, Mark Vogelsberger +10
Understanding how baryonic processes shape the intracluster medium (ICM) is of critical importance to the next generation of galaxy cluster surveys. However, most models of structu…
Imprints of Chameleon f(R) Gravity on Galaxy Rotation Curves
Aneesh P. Naik, Ewald Puchwein, Anne-Christine Davis +1
Current constraints on gravity are relatively weak on galactic and intergalactic scales. Screened modified gravity models can exhibit complex behaviour there without violating stri…