Select Publications
Preprints
, 2024, Everything hot everywhere all at once: Neutrinos and hot dark matter as a single effective species, http://dx.doi.org/10.48550/arxiv.2410.05815
, 2024, One trick to treat them all: SuperEasy linear response for any hot dark matter in $N$-body simulations, http://dx.doi.org/10.48550/arxiv.2410.05816
, 2024, Towards a precision calculation of $N_{\rm eff}$ in the Standard Model III: Improved estimate of NLO contributions to the collision integral, http://dx.doi.org/10.48550/arxiv.2402.18481
, 2023, Cosmic-Enu: An emulator for the non-linear neutrino power spectrum, http://dx.doi.org/10.48550/arxiv.2311.11240
, 2022, Axion minivoids and implications for direct detection, http://dx.doi.org/10.48550/arxiv.2212.00560
, 2022, Flows For The Masses: A multi-fluid non-linear perturbation theory for massive neutrinos, http://dx.doi.org/10.48550/arxiv.2210.16020
, 2022, Hybrid multi-fluid-particle simulations of the cosmic neutrino background, http://dx.doi.org/10.48550/arxiv.2210.16012
, 2022, Gravitational-wave event rates as a new probe for dark matter microphysics, http://dx.doi.org/10.48550/arxiv.2207.14126
, 2022, Probing dark matter interactions with 21cm observations, http://dx.doi.org/10.48550/arxiv.2207.03107
, 2022, Weaker yet again: mass spectrum-consistent cosmological constraints on the neutrino lifetime, http://dx.doi.org/10.48550/arxiv.2203.09075
, 2021, Simulations of axion-like particles in the post-inflationary scenario, http://dx.doi.org/10.48550/arxiv.2112.05117
, 2020, Towards a precision calculation of $N_{\rm eff}$ in the Standard Model II: Neutrino decoupling in the presence of flavour oscillations and finite-temperature QED, http://dx.doi.org/10.48550/arxiv.2012.02726
, 2020, One line to run them all: SuperEasy massive neutrino linear response in $N$-body simulations, http://dx.doi.org/10.48550/arxiv.2011.12504
, 2020, The cosmic neutrino background as a collection of fluids in large-scale structure simulations, http://dx.doi.org/10.48550/arxiv.2011.12503
, 2020, The full Boltzmann hierarchy for dark matter-massive neutrino interactions, http://dx.doi.org/10.48550/arxiv.2011.04206
, 2020, Invisible neutrino decay in precision cosmology, http://dx.doi.org/10.48550/arxiv.2011.01502
, 2020, Spoon or slide? The non-linear matter power spectrum in the presence of massive neutrinos, http://dx.doi.org/10.48550/arxiv.2006.04995
, 2019, Towards a precision calculation of the effective number of neutrinos $N_{\rm eff}$ in the Standard Model I: The QED equation of state, http://dx.doi.org/10.48550/arxiv.1911.04504
, 2019, Fitting functions on the cheap: the relative nonlinear matter power spectrum, http://dx.doi.org/10.48550/arxiv.1907.01125
, 2018, Prior dependence of cosmological constraints on dark matter-radiation interactions, http://dx.doi.org/10.48550/arxiv.1811.11408
, 2018, Trading kinetic energy: How late kinetic decoupling of dark matter changes $N_{\textrm{eff}}$, http://dx.doi.org/10.48550/arxiv.1811.05601
, 2017, CMB spectral distortions as a novel way to probe the small-scale structure problems, http://dx.doi.org/10.48550/arxiv.1710.03121
, 2017, Using CMB spectral distortions to distinguish between dark matter solutions to the small-scale crisis, http://dx.doi.org/10.48550/arxiv.1707.07050
, 2017, Interacting neutrinos in cosmology: exact description and constraints, http://dx.doi.org/10.48550/arxiv.1706.02123
, 2015, Active-sterile neutrino oscillations in the early Universe with full collision terms, http://dx.doi.org/10.48550/arxiv.1506.05266
, 2015, How CMB and large-scale structure constrain chameleon interacting dark energy, http://dx.doi.org/10.48550/arxiv.1505.03154
, 2015, Future cosmological sensitivity for hot dark matter axions, http://dx.doi.org/10.48550/arxiv.1502.03325
, 2014, Higher-order massive neutrino perturbations in large-scale structure, http://dx.doi.org/10.48550/arxiv.1412.2764
, 2014, Getting leverage on inflation with a large photometric redshift survey, http://dx.doi.org/10.48550/arxiv.1409.3469
, 2014, Boltzmann hierarchy for interacting neutrinos I: formalism, http://dx.doi.org/10.48550/arxiv.1409.1577
, 2013, How real-time cosmology can distinguish between different anisotropic models, http://dx.doi.org/10.48550/arxiv.1307.2377
, 2013, Axion hot dark matter bounds after Planck, http://dx.doi.org/10.48550/arxiv.1307.0615
, 2013, Dark energy properties from large future galaxy surveys, http://dx.doi.org/10.48550/arxiv.1304.2321
, 2012, Measuring neutrino masses with a future galaxy survey, http://dx.doi.org/10.48550/arxiv.1209.1043
, 2012, Confronting the sound speed of dark energy with future cluster surveys, http://dx.doi.org/10.48550/arxiv.1205.0548
, 2012, Lagrangian perturbations and the matter bispectrum II: the resummed one-loop correction to the matter bispectrum, http://dx.doi.org/10.48550/arxiv.1203.4261
, 2011, Evidence for dark matter modulation in CoGeNT?, http://dx.doi.org/10.48550/arxiv.1111.3238
, 2011, Sterile neutrinos with eV masses in cosmology -- how disfavoured exactly?, http://dx.doi.org/10.48550/arxiv.1108.4136
, 2011, A Bayesian view of the current status of dark matter direct searches, http://dx.doi.org/10.48550/arxiv.1105.5121
, 2011, Cosmological and Astrophysical Neutrino Mass Measurements, http://dx.doi.org/10.48550/arxiv.1103.5083
, 2010, Spherical collapse of dark energy with an arbitrary sound speed, http://dx.doi.org/10.48550/arxiv.1009.0010
, 2010, Cosmology seeking friendship with sterile neutrinos, http://dx.doi.org/10.48550/arxiv.1006.5276
, 2010, Neutrinos in Non-linear Structure Formation - The Effect on Halo Properties, http://dx.doi.org/10.48550/arxiv.1004.4105
, 2010, Neutrino and axion hot dark matter bounds after WMAP-7, http://dx.doi.org/10.48550/arxiv.1004.0695
, 2010, Cosmological parameters from large scale structure - geometric versus shape information, http://dx.doi.org/10.48550/arxiv.1003.3999
, 2009, Cosmological axion bounds, http://dx.doi.org/10.48550/arxiv.0910.5706
, 2008, Axion hot dark matter bounds, http://dx.doi.org/10.48550/arxiv.0808.0814
, 2008, Observing trans-Planckian ripples in the primordial power spectrum with future large scale structure probes, http://dx.doi.org/10.48550/arxiv.0807.4528
, 2008, Nonlinear corrections to the cosmological matter power spectrum and scale-dependent galaxy bias: implications for parameter estimation, http://dx.doi.org/10.48550/arxiv.0804.1789
, 2008, Cosmological constraints on neutrino plus axion hot dark matter: Update after WMAP-5, http://dx.doi.org/10.48550/arxiv.0803.1585