Ethan E. Uberseder, Ph.D.

Affiliations: 
2013 University of Notre Dame, Notre Dame, IN, United States 
Area:
Radiation Physics, Astrophysics Physics, General Physics
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"Ethan Uberseder"
Mean distance: 14.03
 
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Parents

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Michael C. Wiescher grad student 2013 Notre Dame
 (Experimentally constraining the nucleosynthesis of 60Fe in massive stars.)
Grigory Rogachev post-doc Texas A & M
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Publications

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Upadhyayula S, Rogachev GV, Bishop J, et al. (2020) Search for the high-spin members of the α:2n:α band in Be10 Physical Review C. 101
Heine M, Typel S, Wu MR, et al. (2017) Determination of the neutron-capture rate of C 17 for r -process nucleosynthesis Physical Review C. 95: 14613
Heil M, Plag R, Uberseder E, et al. (2016) Stellar neutron capture cross sections of ⁴¹K and ⁴⁵Sc Physical Review C. 93
Li Q, Görres J, deBoer RJ, et al. (2016) Cross section measurement ofN14(p,γ)O15in the CNO cycle Physical Review C. 93
Uberseder E, Rogachev GV, Goldberg VZ, et al. (2016) Nuclear structure beyond the neutron drip line: The lowest energy states in 9He via their T=5/2 isobaric analogs in 9Li Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics. 754: 323-327
Avila ML, Rogachev GV, Koshchiy E, et al. (2015) Constraining the 6.05 MeV 0+ and 6.13 MeV 3- cascade transitions in the 12C(α,γ)16O reaction using the asymptotic normalization coefficients. Physical Review Letters. 114: 071101
Deboer RJ, Bardayan DW, Görres J, et al. (2015) Low energy scattering cross section ratios of N 14 (p,p) N 14 Physical Review C - Nuclear Physics. 91
Uberseder E, Adachi T, Aumann T, et al. (2014) First experimental constraint on the Fe 59 (n,γ) Fe 60 reaction cross section at astrophysical energies via the coulomb dissociation of Fe 60 Physical Review Letters. 112
Heil M, Plag R, Uberseder E, et al. (2014) Stellar neutron capture cross sections of Ne 20,21,22 Physical Review C - Nuclear Physics. 90
Deboer RJ, Görres J, Smith K, et al. (2014) Monte Carlo uncertainty of the He 3 (α,γ) Be 7 reaction rate Physical Review C - Nuclear Physics. 90
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