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Showing 1-13 of about 13 results.
Galaxy formation with BECDM - II. Cosmic filaments and first galaxiesDOI: info:10.1093/mnras/staa738v. 4942027–2044
Mocz, Philip, Fialkov, Anastasia, Vogelsberger, Mark, Becerra, Fernando, Shen, Xuejian, Robles, Victor H., Amin, Mustafa A., Zavala, Jesús, Boylan-Kolchin, Michael, Bose, Sownak, Marinacci, Federico, Chavanis, Pierre-Henri, Lancaster, Lachlan, and Hernquist, Lars. 2020. "Galaxy formation with BECDM - II. Cosmic filaments and first galaxies." Monthly Notices of the Royal Astronomical Society, 494 2027–2044. https://doi.org/10.1093/mnras/staa738.
Star formation from dense shocked regions in supersonic isothermal magnetoturbulenceDOI: info:10.1093/mnras/sty1976v. 4803916–3927
Mocz, Philip and Burkhart, Blakesley. 2018. "Star formation from dense shocked regions in supersonic isothermal magnetoturbulence." Monthly Notices of the Royal Astronomical Society, 480 3916–3927. https://doi.org/10.1093/mnras/sty1976.
Unveiling the Role of the Magnetic Field at the Smallest Scales of Star FormationDOI: info:10.3847/2041-8213/aa71b7v. 842L9
Hull, Charles L. H., Mocz, Philip, Burkhart, Blakesley, Goodman, Alyssa A., Girart, Josep M., Cortés, Paulo C., Hernquist, Lars, Springel, Volker, Li, Zhi-Yun, and Lai, Shih-Ping. 2017. "Unveiling the Role of the Magnetic Field at the Smallest Scales of Star Formation." The Astrophysical Journal Letters, 842 L9. https://doi.org/10.3847/2041-8213/aa71b7.
Correspondence between constrained transport and vector potential methods for magnetohydrodynamicsDOI: info:10.1016/j.jcp.2016.09.059v. 328221–233
Mocz, Philip. 2017. "Correspondence between constrained transport and vector potential methods for magnetohydrodynamics." Journal of Computational Physics, 328 221–233. https://doi.org/10.1016/j.jcp.2016.09.059.
Moving-mesh Simulations of Star-forming Cores in Magneto-gravo-turbulenceDOI: info:10.3847/1538-4357/aa6475v. 83840
Mocz, Philip, Burkhart, Blakesley, Hernquist, Lars, McKee, Christopher F., and Springel, Volker. 2017. "Moving-mesh Simulations of Star-forming Cores in Magneto-gravo-turbulence." The Astrophysical Journal, 838 40. https://doi.org/10.3847/1538-4357/aa6475.
Mocz, Philip and Succi, Sauro. 2017. "Integer lattice dynamics for Vlasov-Poisson." Monthly Notices of the Royal Astronomical Society, 465 3154–3162. https://doi.org/10.1093/mnras/stw2928.
Galaxy formation with BECDM - I. Turbulence and relaxation of idealized haloesDOI: info:10.1093/mnras/stx1887v. 4714559–4570
Mocz, Philip, Vogelsberger, Mark, Robles, Victor H., Zavala, Jesús, Boylan-Kolchin, Michael, Fialkov, Anastasia, and Hernquist, Lars. 2017. "Galaxy formation with BECDM - I. Turbulence and relaxation of idealized haloes." Monthly Notices of the Royal Astronomical Society, 471 4559–4570. https://doi.org/10.1093/mnras/stx1887.
A moving mesh unstaggered constrained transport scheme for magnetohydrodynamicsDOI: info:10.1093/mnras/stw2004v. 463477–488
Mocz, Philip, Pakmor, Rüdiger, Springel, Volker, Vogelsberger, Mark, Marinacci, Federico, and Hernquist, Lars. 2016. "A moving mesh unstaggered constrained transport scheme for magnetohydrodynamics." Monthly Notices of the Royal Astronomical Society, 463 477–488. https://doi.org/10.1093/mnras/stw2004.
Improving the convergence properties of the moving-mesh code AREPODOI: info:10.1093/mnras/stv2380v. 4551134–1143
Pakmor, Rüdiger, Springel, Volker, Bauer, Andreas, Mocz, Philip, Munoz, Diego J., Ohlmann, Sebastian T., Schaal, Kevin, and Zhu, Chenchong. 2016. "Improving the convergence properties of the moving-mesh code AREPO." Monthly Notices of the Royal Astronomical Society, 455 1134–1143. https://doi.org/10.1093/mnras/stv2380.
The large-scale properties of simulated cosmological magnetic fieldsDOI: info:10.1093/mnras/stv1692v. 4533999–4019
Marinacci, Federico, Vogelsberger, Mark, Mocz, Philip, and Pakmor, Rüdiger. 2015. "The large-scale properties of simulated cosmological magnetic fields." Monthly Notices of the Royal Astronomical Society, 453 3999–4019. https://doi.org/10.1093/mnras/stv1692.
Numerical solution of the nonlinear Schrödinger equation using smoothed-particle hydrodynamicsDOI: info:10.1103/PhysRevE.91.053304v. 91053304
Mocz, Philip and Succi, Sauro. 2015. "Numerical solution of the nonlinear Schrödinger equation using smoothed-particle hydrodynamics." Physical Review E, 91 053304. https://doi.org/10.1103/PhysRevE.91.053304.
Reducing noise in moving-grid codes with strongly-centroidal Lloyd mesh regularizationDOI: info:10.1093/mnras/stv1598v. 4523853–3862
Mocz, Philip, Vogelsberger, Mark, Pakmor, Rüdiger, Genel, Shy, Springel, Volker, and Hernquist, Lars. 2015. "Reducing noise in moving-grid codes with strongly-centroidal Lloyd mesh regularization." Monthly Notices of the Royal Astronomical Society, 452 3853–3862. https://doi.org/10.1093/mnras/stv1598.
A Detection of an X-ray Wind and an Ionized Disk in the Chandra HETGS Observation of the Seyfert 2 Galaxy IRAS 18325-5926DOI: info:10.1088/0004-637X/729/1/30v. 72930
Mocz, Philip, Lee, Julia C., Iwasawa, Kazushi, and Canizares, Claude R. 2011. "A Detection of an X-ray Wind and an Ionized Disk in the Chandra HETGS Observation of the Seyfert 2 Galaxy IRAS 18325-5926." The Astrophysical Journal, 729 30. https://doi.org/10.1088/0004-637X/729/1/30.