Physics – High Energy Physics – High Energy Physics - Experiment
Scientist
Physics
High Energy Physics
High Energy Physics - Experiment
Scientist
University of Maryland
School of Mathematical Sciences, University of Exeter, EX4 4QJ, UK
Bullard Laboratory, Department of Earth Sciences, University of Cambridge
SPACE Research Centre, RMIT University, Melbourne, VIC, Australia; of Mathematical Sciences, University of Exeter, EX4 4QE, UK
Department of Mathematics, University of Exeter, Exeter, UK
The School of Mathematical Sciences, University of Exeter, Exeter, UK
Brookhaven National Laboratory, Upton, New York, USA
University of California Santa Cruz, 1156 High Street, Santa Cruz, CA 95064, USA Physikalisches Institut, Universität Göttingen, Friedrich-Hund-Platz 1, D-37077 Göttingen, Germany
Department of Earth Sciences, University of Leeds, Leeds LS2 9JT, UK
Center for Geophysical and Astrophysical Fluid Dynamics, and Department of Mathematical Sciences, University of Exeter, Exeter EX4 4QE, UK
University of Exeter, Department of Mathematical Sciences, Exeter, United Kingdom
University of Exeter, Department of Mathematical Sciences, Exeter, EX4 4QE, United Kingdom of Mathematics, University of Exeter, Exeter EX4 4QE, UK
Department of Mathematical Sciences, College of Engineering, Mathematics and Physical Sciences, University of Exeter, Exeter, UK
Department of Mathematics, University of Exeter
RMIT SPACE Research Centre, RMIT University, Melbourne, Australia; Tel.: +61 3 9925 3272; fax: +61 3 9663 2517.
Department of Mathematics, University of Exeter, EX4 4QE, Exeter, UK
School of Mathematical Sciences, University of Exeter, North Park Road, Exeter, EX4 4QE United Kingdom for Geophysical and Astrophysical Fluid Dynamics and Department of Mathematical Sciences, University of Exeter, EX4 4QE, UK.
Mathematics, University of Exeter, Exeter, United Kingdom
Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China; School of Mathematical Sciences, Un
$K^{*0}$ and $Σ^*$ production in Au+Au collisions at $\sqrt{s_{NN}}=$ 200 GeV and 62.4 GeV
A Monte Carlo Approach for Studying Microphases Applied to the Axial Next-Nearest-Neighbor Ising and the Ising-Coulomb Models
A Multi-object Exoplanet Detecting Technique
A numerical dynamo benchmark
A Sandwich Interface Dynamo: Linear Dynamo Waves in the Sun
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