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papers

Publications (18)

astro-ph.CO2011

The inverse-Compton ghost HDF 130 and the giant radio galaxy 6C 0905+3955: matching an analytic model for double radio source evolution

Philip Mocz, A. C. Fabian, Katherine M. Blundell +3

astro-ph.IM2015

Reducing noise in moving-grid codes with strongly-centroidal Lloyd mesh regularization

Philip Mocz, Mark Vogelsberger, Rudiger Pakmor +3

astro-ph.CO2012

The Tully-Fisher Relation for 25,000 SDSS Galaxies as Function of Environment

Philip Mocz, Andrew Green, Max Malacari +1

astro-ph.IM2016

A moving mesh unstaggered constrained transport scheme for magnetohydrodynamics

Philip Mocz, Ruediger Pakmor, Volker Springel +3

astro-ph.HE2011

A Detection of an X-ray Wind and an Ionized Disk in the Chandra HETGS Observation of the Seyfert 2 Galaxy IRAS 18325-5926

Philip Mocz, Julia C. Lee, Kazushi Iwasawa +1

astro-ph.CO2018

On the Schrodinger-Poisson--Vlasov-Poisson correspondence

Philip Mocz, Lachlan Lancaster, Anastasia Fialkov +2

astro-ph.IM2014

A Constrained Transport Scheme for MHD on Unstructured Static and Moving Meshes

Philip Mocz, Mark Vogelsberger, Lars Hernquist

astro-ph.HE2014

Interpreting MAD within multiple accretion regimes

Philip Mocz, Xinyi Guo

astro-ph.GA2017

Moving mesh simulations of star forming cores in magneto-gravo-turbulence

Philip Mocz, Blakesley Burkhart, Lars Hernquist +2

astro-ph.GA2016

Integer Lattice Dynamics for Vlasov-Poisson

Philip Mocz, Sauro Succi

astro-ph.GA2017

Unveiling the Role of the Magnetic Field at the Smallest Scales of Star Formation

Charles L. H. Hull, Philip Mocz, Blakesley Burkhart +7

astro-ph.GA2015

Improving the convergence properties of the moving-mesh code AREPO

Ruediger Pakmor, Volker Springel, Andreas Bauer +5

astro-ph.CO2015

The large-scale properties of simulated cosmological magnetic fields

Federico Marinacci, Mark Vogelsberger, Philip Mocz +1

astro-ph.IM2018

Non-ideal magnetohydrodynamics on a moving mesh

Federico Marinacci, Mark Vogelsberger, Rahul Kannan +3

physics.comp-ph2016

Numerical solution of the non-linear Schrodinger equation using smoothed-particle hydrodynamics

Philip Mocz, Sauro Succi

astro-ph.HE2018

Evolution of the Black Hole Mass Function in Star Clusters from Multiple Mergers

Pierre Christian, Philip Mocz, Abraham Loeb

astro-ph.GA2018

Star formation from dense shocked regions in supersonic isothermal magneto-turbulence

Philip Mocz, Blakesley Burkhart

astro-ph.CO2017

Galaxy Formation with BECDM: I. Turbulence and relaxation of idealised haloes

Philip Mocz, Mark Vogelsberger, Victor Robles +4