1 code implementation • 3 Nov 2022 • Jonas El Gammal, Nils Schöneberg, Jesús Torrado, Christian Fidler
GPry does not need any pre-training, special hardware such as GPUs, and is intended as a drop-in replacement for traditional Monte Carlo methods for Bayesian inference.
no code implementations • 12 Jul 2019 • Jasper Albers, Christian Fidler, Julien Lesgourgues, Nils Schöneberg, Jesus Torrado
Einstein-Boltzmann Solvers (EBSs) are run on a massive scale by the cosmology community when fitting cosmological models to data.
Cosmology and Nongalactic Astrophysics
1 code implementation • 24 Nov 2015 • Christian Fidler, Guido Pettinari, Cyril Pitrou
Since scalar perturbations do not generate any magnetic field as they are curl-free, one has to resort to second-order perturbation theory to compute the magnetic field generated by this effect.
Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies General Relativity and Quantum Cosmology
1 code implementation • 11 Jun 2014 • Guido W. Pettinari, Christian Fidler, Robert Crittenden, Kazuya Koyama, Antony Lewis, David Wands
We find that the presence of the intrinsic bispectrum will bias a measurement of primordial non-Gaussianity of local type by $f_{NL}^\text{bias}=0. 66$ for an ideal experiment with $\ell_\text{max}=3000$.
Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology
no code implementations • 14 Jan 2014 • Christian Fidler, Guido W. Pettinari, Martin Beneke, Robert Crittenden, Kazuya Koyama, David Wands
The intrinsic B-mode polarisation is present independent of the initial conditions and might contaminate the signal from primordial gravitational waves.
Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology
no code implementations • 16 Dec 2013 • Sebastien Renaux-Petel, Christian Fidler, Cyril Pitrou, Guido W. Pettinari
We find that $B$-modes are of the same order of magnitude as $E$-modes.
Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology
1 code implementation • 4 Feb 2013 • Guido W. Pettinari, Christian Fidler, Robert Crittenden, Kazuya Koyama, David Wands
We develop a new, efficient code for solving the second-order Einstein-Boltzmann equations, and use it to estimate the intrinsic CMB non-Gaussianity arising from the non-linear evolution of density perturbations.
Cosmology and Nongalactic Astrophysics High Energy Physics - Theory