226 results on '"Fryer, Chris"'
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2. Fundamental physics studies in time domain and multi-messenger astronomy
3. A lanthanide-rich kilonova in the aftermath of a long gamma-ray burst
4. The Effect of the Velocity Distribution on Kilonova Emission
5. The High Energy X-ray Probe (HEX-P): supernova remnants, pulsar wind nebulae, and nuclear astrophysics
6. The high energy X-ray probe (HEX-P): Galactic PeVatrons, star clusters, superbubbles, microquasar jets, and gamma-ray binaries
7. Interpolated kilonova spectra models: Examining the effects of a phenomenological, blue component in the fitting of AT2017gfo spectra
8. Heavy element production in a compact object merger observed by JWST
9. Constraining Inputs to Realistic Kilonova Simulations through Comparison to Observed r-process Abundances
10. Abundances and Transients from Neutron Star–White Dwarf Mergers
11. Lagrangian large eddy simulations via physics-informed machine learning
12. The Compton Spectrometer and Imager
13. A lanthanide-rich kilonova in the aftermath of a long gamma-ray burst
14. Particle-in-cell Simulations of Mildly Relativistic Outflows in Kilonova Emissions
15. JWST detection of heavy neutron capture elements in a compact object merger
16. Neutron Star Binaries Produced by Binary-Driven Hypernovae, Their Mergers, and the Link between Long and Short GRBs
17. Finding My Drumbeat: Applying Lessons Learned from Remo Ruffini to Understanding Astrophysical Transients
18. Physics-informed machine learning with smoothed particle hydrodynamics: Hierarchy of reduced Lagrangian models of turbulence
19. Astrophysics with the Laser Interferometer Space Antenna
20. Probes of the progenitors, engines and physics behind stellar collapse
21. Evolution of Accreting Neutron Star Common Envelopes and Their Nucleosynthesis Possible P-nuclide Production
22. Short GRB Host Galaxies. I. Photometric and Spectroscopic Catalogs, Host Associations, and Galactocentric Offsets
23. Physics-informed Machine Learning for Modeling Turbulence in Supernovae
24. All-sky Medium Energy Gamma-ray Observatory eXplorer mission concept
25. The role of supernova convection for the lower mass gap in the isolated binary formation of gravitational wave sources
26. Inferring the temperature profile of the radiative shock in the COAX experiment with shock radiography, Dante, and spectral temperature diagnostics
27. Catching Element Formation In The Act - The Case for a New MeV Gamma-Ray Mission: Radionuclide Astronomy in the 2020s
28. An Isolated Stellar-mass Black Hole Detected through Astrometric Microlensing*
29. The Effect of Supernova Convection On Neutron Star and Black Hole Masses
30. Supernova Shock Breakout/Emergence Detection Predictions for a Wide-field X-Ray Survey
31. Properties of High-redshift Gamma-Ray Bursts
32. Probes of the progenitors, engines and physics behind stellar collapse
33. Radioactive nuclei in the early Solar system: analysis of the 15 isotopes produced by core-collapse supernovae
34. Sapsan: Framework for Supernovae Turbulence Modeling with Machine Learning
35. Sensitivity of Neutron-Rich Nuclear Isomer Behavior to Uncertainties in Direct Transitions
36. Nuclear Physics Exascale Requirements Review: An Office of Science review sponsored jointly by Advanced Scientific Computing Research and Nuclear Physics, June 15 - 17, 2016, Gaithersburg, Maryland
37. Transport of Protostellar Cosmic Rays in Turbulent Dense Cores
38. Cosmic ray transport in mixed magnetic fields and their role on the observed anisotropies
39. Finishing Mill Predictive Temperature Control
40. The Impact of Nuclear Physics Uncertainties on Galactic Chemical Evolution Predictions
41. The Role of Inhomogeneities in Supernova Shock Breakout Emission
42. Compact Remnant Constraints on the Core-Collapse Engine
43. The Collapsar Engine for GRBS and Hypernovae
44. Stellar Collapse and Gravitational Waves
45. Population Synthesis and Gamma-Ray Burst Progenitors
46. Low Mass SN Ia and the Late Light Curve
47. Understanding the engines and progenitors of gamma-ray bursts
48. Impact of Pulsar and Fallback Sources on Multifrequency Kilonova Models
49. Neutron Star Mergers Might Not Be the Only Source of r-process Elements in the Milky Way
50. A luminosity distribution for kilonovae based on short gamma-ray burst afterglows
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