2023 |
**M. Mumpower**, M. Li, T. M. Sprouse, B. S. Meyer, *et al.* |
Bayesian averaging for ground state masses of atomic nuclei in a Machine Learning approach |
submitted |

2023 |
E. Holmbeck, J. Barnes, K. Lund, T. M. Sprouse, *et al.* |
Superheavy elements in kilonovae |
submitted |

2023 |
S. Curtis, J. Miller, C. Frohlich, T. M. Sprouse, *et al.* |
Nucleosynthesis in outflows from black hole-neutron star merger disks with full GR$\nu$RMHD |
ApJL 945 L13 |

2023 |
E. Holmbeck, T. M. Sprouse, **M. Mumpower** |
Nucleosynthesis and observation of the heaviest elements |
EPJA 59 28 |

2022 |
**M. Mumpower**, T. Kawano, T. M. Sprouse |
$\beta^{-}$-delayed fission in the coupled Quasi-particle Random Phase Approximation plus Hauser-Feshbach approach |
PRC 106 065805 |

2022 |
C. J. Fontes, C. L. Fryer, R. T. Wollaeger, **M. Mumpower**, *et al.* |
Actinide opacities for modeling the spectra and light curves of kilonovae |
MNRAS stac2792 |

2022 |
**M. Mumpower**, T. M. Sprouse, A. Lovell, A. T. Mohan |
Physically Interpretable Machine Learning for nuclear masses |
PRCL 106 021301 |

2022 |
A. Lovell, A. T. Mohan, T. M. Sprouse, **M. Mumpower** |
Nuclear masses learned from a probabilistic neural network |
PRC 106 014305 |

2022 |
M. Ristic, E. Holmbeck, R. T. Wollaeger, O. Korobkin, *et al.* |
Constraining inputs to realistic kilonova simulations through comparison to observed $r$-process abundances |
submitted |

2022 |
H. F. Li, S. Naimi, T. M. Sprouse, **M. Mumpower**, *et al.* |
First application of mass measurement with the Rare-RI Ring reveals the solar $r$-process abundance trend at $A=122$ and $A=123$ |
PRL 128 152701 |

2022 |
T. M. Sprouse, G. W. Misch, **M. Mumpower** |
Isochronic evolution and the radioactive decay of $r$-process nuclei |
ApJ 929 22 |

2021 |
G. W. Misch, T. M. Sprouse, **M. Mumpower**, A. J. Couture, *et al.* |
Sensitivity of neutron-rich nuclear isomer behavior to uncertainties in direct transitions |
Symmetry 13 1831 |

2021 |
J. Barnes, Y. Zhu, K. Lund, T. M. Sprouse, *et al.* |
Kilonovae across the nuclear physics landscape: the impact of nuclear physics uncertainties on r-process-powered emission |
ApJ 918 44 |

2021 |
T. M. Sprouse, **M. Mumpower**, R. Surman |
Following nuclei through nucleosynthesis: a novel tracing technique |
PRC 104 015803 |

2021 |
G. W. Misch, T. M. Sprouse, **M. Mumpower** |
Astromers in the radioactive decay of r-process nuclei |
ApJL 913 L2 |

2021 |
E. Holmbeck, A. Frebel, G. C. McLaughlin, R. Surman, *et al.* |
Reconstructing masses of merging neutron stars from stellar r-process abundance signatures |
ApJ 909 21 |

2021 |
B. Côtè, M. Eichler, A. Yague, N. Vassh, *et al.* |
Constraining the rapid neutron-capture process with meteoritic 129-I and 247-Cm |
Science 371 945-948 |

2021 |
Y. Zhu, K. Lund, J. Barnes, T. M. Sprouse, *et al.* |
Modeling kilonova light curves: dependence on nuclear inputs |
ApJ 906 94 |

2020 |
X. Wang, N. Vassh, T. M. Sprouse, **M. Mumpower**, *et al.* |
MeV gamma rays from fission: a distinct signature of actinide production in neutron star mergers |
ApJL 903 1 |

2020 |
J. Miller, T. M. Sprouse, C. L. Fryer, B. R. Ryan, *et al.* |
Full transport general relativistic radiation magnetohydrodynamics for nucleosynthesis in collapsars |
ApJ 902 1 |

2020 |
N. Vassh, **M. Mumpower**, G. C. McLaughlin, T. M. Sprouse, *et al.* |
Co-production of light and heavy $r$-process elements via fission deposition |
ApJ 896 1 |

2020 |
T. M. Sprouse, R. Navarro Perez, R. Surman, **M. Mumpower**, *et al.* |
Propagation of statistical uncertainties of Skyrme mass models to simulations of $r$-process nucleosynthesis |
PRC 101 055803 |

2020 |
X. Wang, B. D. Fields, **M. Mumpower**, T. M. Sprouse, *et al.* |
Sandblasting the $r$-process: spallation of ejecta from neutron star mergers |
ApJ 893 2 |

2020 |
J. Wu, S. Nishimura, P. Möller, **M. Mumpower**, *et al.* |
$\beta$-decay half-lives of 55 neutron-rich isotopes beyond the $N=82$ shell gap |
PRC rapid communication |

2020 |
O. Korobkin, A. Hungerford, C. L. Fryer, **M. Mumpower**, *et al.* |
Gamma-rays from kilonova: a potential probe of r-process nucleosynthesis |
ApJ 889 2 |

2019 |
E. Holmbeck, A. Frebel, G. C. McLaughlin, **M. Mumpower**, *et al.* |
Actinide-rich and actinide-poor r-process enhanced metal-poor stars do not require separate r-process progenitors |
ApJ 881 1 |

2019 |
N. Vassh, R. Vogt, R. Surman, J. Randrup, *et al.* |
Using excitation-energy dependent fission yields to identify key fissioning nuclei in r-process nucleosynthesis |
J. Phys. G 46 065202 |

2018 |
E. Holmbeck, R. Surman, T. M. Sprouse, **M. Mumpower**, *et al.* |
Actinide production in neutron-rich ejecta of a neutron star merger |
ApJ 870 1 |

2018 |
**M. Mumpower**, T. Kawano, T. M. Sprouse, N. Vassh, *et al.* |
$\beta$-delayed fission in $r$-process nucleosynthesis |
ApJ 869 1 |

2018 |
A. Aprahamian, R. Surman, A. Frebel, G. C. McLaughlin, *et al.* |
FRIB and the GW170817 kilonova |
Whitepaper |

2018 |
Y. Zhu, R. T. Wollaeger, N. Vassh, R. Surman, *et al.* |
Californium-254 and kilonova light curves |
ApJL 863 2 |

2018 |
B. Côtè, C. L. Fryer, K. Belczynski, O. Korobkin, *et al.* |
The origin of r-process elements in the Milky Way |
ApJ 855 2 |

2017 |
**M. Mumpower**, T. Kawano, J. L. Ullmann, M. Krticka, *et al.* |
Estimation of M1 scissors mode strength for deformed nuclei in the medium to heavy mass region by statistical Hauser-Feshbach model calculations |
PRC 96 024612 |