no code implementations • 11 Feb 2021 • C. Wellenhofer, C. Drischler, A. Schwenk
We discuss high-order calculations in perturbative effective field theory for fermions at low energy scales.
Quantum Gases High Energy Physics - Phenomenology Nuclear Theory
no code implementations • 5 Jan 2021 • C. Drischler, J. W. Holt, C. Wellenhofer
Born in the aftermath of core collapse supernovae, neutron stars contain matter under extraordinary conditions of density and temperature that are difficult to reproduce in the laboratory.
Nuclear Theory High Energy Astrophysical Phenomena Solar and Stellar Astrophysics High Energy Physics - Phenomenology Nuclear Experiment
1 code implementation • 10 Sep 2020 • R. Somasundaram, C. Drischler, I. Tews, J. Margueron
The nuclear symmetry energy is a key quantity in nuclear (astro)physics.
Nuclear Theory
1 code implementation • 16 Apr 2020 • C. Drischler, J. A. Melendez, R. J. Furnstahl, D. R. Phillips
The inferred in-medium $\chi$EFT breakdown scale in pure neutron matter and symmetric nuclear matter is consistent with that from free-space nucleon-nucleon scattering.
Nuclear Theory High Energy Astrophysical Phenomena High Energy Physics - Phenomenology Nuclear Experiment
1 code implementation • 15 Apr 2020 • C. Drischler, R. J. Furnstahl, J. A. Melendez, D. R. Phillips
We introduce a new framework for quantifying correlated uncertainties of the infinite-matter equation of state derived from chiral effective field theory ($\chi$EFT).
Nuclear Theory High Energy Astrophysical Phenomena High Energy Physics - Phenomenology Nuclear Experiment
