Search Results - "Holmbeck, E."

β-delayed Fission in r-process Nucleosynthesis by Mumpower, M. R., Kawano, T., Sprouse, T. M., Vassh, N., Holmbeck, E. M., Surman, R., Möller, P.

“…We present β-delayed neutron emission and β-delayed fission (βdf) calculations for heavy, neutron-rich nuclei using the coupled Quasi-Particle Random Phase…”
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Nucleosynthesis and observation of the heaviest elements by Holmbeck, E. M., Sprouse, T. M., Mumpower, M. R.

“…The rapid neutron capture or ‘ r process’ of nucleosynthesis is believed to be responsible for the production of approximately half the natural abundance of…”
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Nucleosynthesis and observation of the heaviest elements by Holmbeck, E. M, Sprouse, T. M, Mumpower, M. R

“…European Physical Journal A, 59, 28 (2023) The rapid neutron capture or 'r process' of nucleosynthesis is believed to be responsible for the production of…”
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Medication Adherence in Patients with Hematologic Malignancies Who Are Hematopoietic Stem Cell Transplantation Survivors: A Qualitative Study by Amonoo, Hermioni L., Deary, Emma C., Wang, Annie, Newcomb, Richard A., Daskalakis, Elizabeth, Weber, Daniel, Holmbeck, Katherine E., Choe, Joanna J., Nabily, Anisa, Cutler, Corey, Traeger, Lara N., El-Jawahri, Areej

“…•Patients describe medication adherence as taking medications on the prescribed day, irrespective of the prescribed time.•Medication quantity and side effects…”
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The r-Process Pattern of a Bright, Highly r-Process-Enhanced, Metal-Poor Halo Star at [Fe/H] ~ -2 by Sakari, C. M, Placco, V. M, Hansen, T, Holmbeck, E. M, Beers, T. C, Frebel, A, Roederer, I. U, Venn, K. A, Wallerstein, G, Davis, C. E, Farrell, E. M, Yong, D

“…A high-resolution spectroscopic analysis is presented for a new highly r-process-enhanced ([Eu/Fe] = 1.27, [Ba/Eu] = -0.65), very metal-poor ([Fe/H] = -2.09),…”
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Californium-254 and kilonova light curves by Zhu, Y, Wollaeger, R. T, Vassh, N, Surman, R, Sprouse, T. M, Mumpower, M. R, Moller, P, McLaughlin, G. C, Korobkin, O, Kawano, T, Jaffke, P. J, Holmbeck, E. M, Fryer, C. L, Even, W. P, Couture, A. J, Barnes, J

“…Neutron star mergers offer unique conditions for the creation of the heavy elements and additionally provide a testbed for our understanding of this synthesis…”
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HR-GO I: Comprehensive NLTE abundance analysis of the Cetus stream by Sitnova, T. M, Yuan, Z, Matsuno, T, Mashonkina, L. I, Alexeeva, S. A, Holmbeck, E, Sestito, F, Lombardo, L, Banerjee, P, Martin, N. F, Jiang, F

“…Dwarf galaxy streams encode vast amounts of information essential to understanding early galaxy formation and nucleosynthesis channels. Due to the variation in…”
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The R-Process Alliance: Analysis of Limited-r Stars by Xylakis-Dornbusch, T, Hansen, T. T, Beers, T. C, Christlieb, N, Ezzeddine, R, Frebel, A, Holmbeck, E, Placco, V. M, Roederer, I. U, Sakari, C. M, Sneden, C

“…Context. In recent years, the R-Process Alliance (RPA) has conducted a successful search for stars enhanced in elements produced by the rapid neutron-capture…”
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Constraining inputs to realistic kilonova simulations through comparison to observed $r$-process abundances by Ristic, M, Holmbeck, E. M, Wollaeger, R, Korobkin, O, Champion, E, O'Shaughnessy, R, Fryer, C. L, Fontes, C. J, Mumpower, M. R, Sprouse, T. M

“…Kilonovae, one source of electromagnetic emission associated with neutron star mergers, are powered by the decay of radioactive isotopes in the neutron-rich…”
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beta$-delayed fission in $r$-process nucleosynthesis by Mumpower, M. R, Kawano, T, Sprouse, T. M, Vassh, N, Holmbeck, E. M, Surman, R, Moller, P

“…We present $\beta$-delayed neutron emission and $\beta$-delayed fission calculations for heavy, neutron-rich nuclei using the coupled Quasi-Particle Random…”
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Horizons: Nuclear Astrophysics in the 2020s and Beyond by Schatz, H, Best, A, Chatziioannou, K, Deibel, C. M, Ezzeddine, R, Lugaro, M, Meisel, Z, Norman, D, Roberts, L. F, Tews, I, Timmes, F. X, Travaglio, C, Abia, C, Agarwal, S, Aoki, W, Arcones, A, Aryan, A, Bandyopadhyay, A, Barnes, J, Bauswein, A, Bishop, J, Caplan, M. E, Champagne, A. E, Couder, M, Couture, A, Debnath, S, deBoer, R. J, Hartogh, J. den, Denissenkov, P, Dexheimer, V, Escher, J. E, Farmer, R, Fisher, R, Frebel, A, Fuller, G, Gibson, B. K, Gourgouliatos, K. N, Graber, V, Gupta, M, Haxton, W, Heger, A, Hix, W. R, Holmbeck, E. M, Huth, S, Imbriani, G, Izzard, R. G, Kajino, T, Kankainen, A, Kiss, G. G, La Cognata, M, Lamia, L, Laplace, E, Launey, K. D, Leckenby, G, Lennarz, A, Lovell, A. E, Lyons, S. M, Maeda, K, Merc, J, Mumpower, M, Neto, D, Nishikawa, K, Nishimura, N, Nunes, F. M, O'Connor, E, O'Shea, B. W, Pain, S. D, Pajkos, M. A, Pizzone, R. G, Placco, V. M, Plewa, T, Pritychenko, B, Psaltis, A, Puentes, D, Qian, Y-Z, Reifarth, R, Richard, A. L, Roederer, I. U, K, J. S, Saito, Y, Schwenk, A, Sergi, M. L, Sidhu, R. S, Simon, A, Sivarani, T, Skúladóttir, Á, Sprouse, T. M, Steiner, A. W, Strieder, F, Sultana, I, Tawfik, A, Tsang, M. B, Tumino, A, Upadhyayula, S, Martínez, J. O. Valle, Vázquez, C. Viscasillas, Wehmeyer, B, Wrede, C, Yoon, J, Zermane, M. A

“…Nuclear Astrophysics is a field at the intersection of nuclear physics and astrophysics, which seeks to understand the nuclear engines of astronomical objects…”
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