Search Results - "Pfrommer, C."

Cosmic-ray hydrodynamics: Alfvén-wave regulated transport of cosmic rays by Thomas, T, Pfrommer, C

“…ABSTRACT Star formation in galaxies appears to be self-regulated by energetic feedback processes. Among the most promising agents of feedback are cosmic rays…”
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Simulations of the dynamics of magnetized jets and cosmic rays in galaxy clusters by Ehlert, K, Weinberger, R, Pfrommer, C, Pakmor, R, Springel, V

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Comparing different closure relations for cosmic ray hydrodynamics by Thomas, T, Pfrommer, C

“…ABSTRACT Cosmic ray (CR) hydrodynamics is a (re-)emerging field of high interest due to the importance of CRs for the dynamical evolution of the interstellar,…”
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Simulating cosmic ray physics on a moving mesh by Pfrommer, C, Pakmor, R, Schaal, K, Simpson, C M, Springel, V

“…We discuss new methods to integrate the cosmic ray (CR) evolution equations coupled to magnetohydrodynamics on an unstructured moving mesh, as realized in the…”
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A finite volume method for two-moment cosmic ray hydrodynamics on a moving mesh by Thomas, T, Pfrommer, C, Pakmor, R

“…ABSTRACT We present a new numerical algorithm to solve the recently derived equations of two-moment cosmic ray hydrodynamics (CRHD). The algorithm is…”
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Draping of Cluster Magnetic Fields over Bullets and Bubbles—Morphology and Dynamic Effects by Dursi, L. J, Pfrommer, C

“…High-resolution X-ray observations have revealed cavities and 'cold fronts' with sharp edges in temperature and density within galaxy clusters. Their presence…”
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Cosmic-ray-driven galactic winds: transport modes of cosmic rays and Alfvén-wave dark regions by Thomas, T, Pfrommer, C, Pakmor, R

“…ABSTRACT Feedback mediated by cosmic rays (CRs) is an important process in galaxy formation. Because CRs are long-lived and because they are transported along…”
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ON THE CLUSTER PHYSICS OF SUNYAEV―ZEL'DOVICH AND X-RAY SURVEYS. II. DECONSTRUCTING THE THERMAL SZ POWER SPECTRUM by BATTAGLIA, N, BOND, J. R, PFROMMER, C, SIEVERS, J. L

“…Secondary anisotropies in the cosmic microwave background are a treasure-trove of cosmological information. Interpreting current experiments probing them are…”
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The effect of cosmic ray acceleration on supernova blast wave dynamics by Pais, M, Pfrommer, C, Ehlert, K, Pakmor, R

“…ABSTRACT Non-relativistic shocks accelerate ions to highly relativistic energies provided that the orientation of the magnetic field is closely aligned with…”
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Galactic winds driven by cosmic ray streaming by Uhlig, M., Pfrommer, C., Sharma, M., Nath, B. B., Enßlin, T. A., Springel, V.

“…Galactic winds are observed in many spiral galaxies with sizes from dwarfs up to the Milky Way, and they sometimes carry a mass in excess of that of newly…”
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ON THE CLUSTER PHYSICS OF SUNYAEV―ZEL'DOVICH AND X-RAY SURVEYS. I. THE INFLUENCE OF FEEDBACK, NON-THERMAL PRESSURE, AND CLUSTER SHAPES ON Y―M SCALING RELATIONS by BATTAGLIA, N, BOND, J. R, PFROMMER, C, SIEVERS, J. L

“…The utility of large Sunyaev-Zel'dovich (SZ) surveys for determining cosmological parameters from cluster abundances is limited by the theoretical…”
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Self-regulated AGN feedback of light jets in cool-core galaxy clusters by Ehlert, K, Weinberger, R, Pfrommer, C, Pakmor, R, Springel, V

“…ABSTRACT Heating from active galactic nuclei (AGNs) is thought to stabilize cool-core clusters, limiting star formation and cooling flows. We employ radiative…”
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ON THE CLUSTER PHYSICS OF SUNYAEV-ZEL'DOVICH AND X-RAY SURVEYS. III. MEASUREMENT BIASES AND COSMOLOGICAL EVOLUTION OF GAS AND STELLAR MASS FRACTIONS by Battaglia, N, Bond, J R, Pfrommer, C, Sievers, J L

“…Gas masses tightly correlate with the virial masses of galaxy clusters, allowing for a precise determination of cosmological parameters by means of X-ray…”
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Connecting turbulent velocities and magnetic fields in galaxy cluster simulations with active galactic nuclei jets by Ehlert, K, Weinberger, R, Pfrommer, C, Springel, V

“…ABSTRACT The study of velocity fields of the hot gas in galaxy clusters can help to unravel details of microphysics on small scales and to decipher the nature…”
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Non-Kolmogorov turbulence in multiphase intracluster medium driven by cold gas precipitation and AGN jets by Wang, C, Ruszkowski, M, Pfrommer, C, Oh, S Peng, Yang, H-Y K

“…ABSTRACT Active galactic nuclei (AGNs) feedback is responsible for maintaining plasma in global thermal balance in extended haloes of elliptical galaxies and…”
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Simulations of the Sunyaev-Zel'dovich Power Spectrum with Active Galactic Nucleus Feedback by Battaglia, N, Bond, J. R, Pfrommer, C, Sievers, J. L, Sijacki, D

“…We explore how radiative cooling, supernova feedback, cosmic rays, and a new model of the energetic feedback from active galactic nuclei (AGNs) affect the…”
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Whistler-regulated Magnetohydrodynamics: Transport Equations for Electron Thermal Conduction in the High-β Intracluster Medium of Galaxy Clusters by Drake, J. F., Pfrommer, C., Reynolds, C. S., Ruszkowski, M., Swisdak, M., Einarsson, A., Thomas, T., Hassam, A. B., Roberg-Clark, G. T.

“…Abstract Transport equations for electron thermal energy in the high- β e intracluster medium (ICM) are developed that include scattering from both classical…”
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A comparison of cosmological codes: properties of thermal gas and shock waves in large-scale structures by Vazza, F., Dolag, K., Ryu, D., Brunetti, G., Gheller, C., Kang, H., Pfrommer, C.

“…Cosmological hydrodynamical simulations are a valuable tool for understanding the growth of large-scale structure and the observables connected with this. Yet,…”
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Detecting shock waves in cosmological smoothed particle hydrodynamics simulations by Pfrommer, C., Springel, V., Enßlin, T. A., Jubelgas, M.

“…We develop a formalism for the identification and accurate estimation of the strength of structure formation shocks during cosmological smoothed particle…”
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ON THE CLUSTER PHYSICS OF SUNYAEV-ZEL'DOVICH AND X-RAY SURVEYS. IV. CHARACTERIZING DENSITY AND PRESSURE CLUMPING DUE TO INFALLING SUBSTRUCTURES by Battaglia, N., Bond, J. R., Pfrommer, C., Sievers, J. L.

“…ABSTRACT Understanding the outskirts of galaxy clusters at the virial radius (R200) and beyond is critical for an accurate determination of cluster masses,…”
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