C
C. Drischler
Researcher at Michigan State University
Publications - 32
Citations - 1581
C. Drischler is an academic researcher from Michigan State University. The author has contributed to research in topics: Effective field theory & Nuclear matter. The author has an hindex of 14, co-authored 25 publications receiving 1012 citations. Previous affiliations of C. Drischler include Lawrence Berkeley National Laboratory & Technische Universität Darmstadt.
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Journal ArticleDOI
Neutron and weak-charge distributions of the 48Ca nucleus
Gaute Hagen,Gaute Hagen,Andreas Ekström,Andreas Ekström,Christian Forssén,Christian Forssén,Christian Forssén,Gustav R. Jansen,Gustav R. Jansen,Witold Nazarewicz,Witold Nazarewicz,Witold Nazarewicz,Thomas Papenbrock,Thomas Papenbrock,K. A. Wendt,K. A. Wendt,Sonia Bacca,Sonia Bacca,Nir Barnea,B. D. Carlsson,C. Drischler,Kai Hebeler,Morten Hjorth-Jensen,Morten Hjorth-Jensen,Mirko Miorelli,Mirko Miorelli,Giuseppina Orlandini,Giuseppina Orlandini,Achim Schwenk,J. Simonis +29 more
TL;DR: In this article, an ab initio calculation of the neutron distribution of the Neutron-rich nucleus Ca-48 is presented, and it is shown that the difference between the radii of the neutrons and proton distributions is significantly smaller than previously thought.
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Chiral interactions up to next-to-next-to-next-to-leading order and nuclear saturation
TL;DR: An efficient Monte Carlo framework for perturbative calculations of infinite nuclear matter based on chiral two-, three-, and four-nucleon interactions is presented, demonstrating a very good many-body convergence up to fourth order and exploring new chiral interactions up to N^{3}LO.
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How Well Do We Know the Neutron-Matter Equation of State at the Densities Inside Neutron Stars? A Bayesian Approach with Correlated Uncertainties.
TL;DR: This work introduces a new framework for quantifying correlated uncertainties of the infinite-matter equation of state derived from chiral effective field theory (χEFT), and produces the first statistically robust uncertainty estimates for key quantities of neutron stars.
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Asymmetric nuclear matter based on chiral two- and three-nucleon interactions
TL;DR: In this paper, the properties of isospin-asymmetric nuclear matter based on chiral nucleon-nucleon (NN) and 3N interactions were calculated and an improved normal-ordering framework was developed.
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Neutron matter from chiral two- and three-nucleon calculations up to N$^3$LO
TL;DR: In this paper, the authors used the partial-wave decomposition of three-nucleon forces in the chiral effective field theory (EFT) to provide improved predictions for the equation of state of neutron matter at zero temperature and analyzed the many-body convergence for different chiral EFT interactions.