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Variational Monte Carlo calculations of n + H 3 scattering

Physical review. C, 2023-09, Vol.108 (3), Article 034001

2023

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S -factor and scattering-parameter extractions from ^{3}\mathrm{He}+{}^{4}\mathrm{He}{ \rightarrow }^{7}\mathrm{Be}+\gamma

Journal of physics. G, Nuclear and particle physics, 2020-05, Vol.47 (5), p.54002

2020

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S-factor and scattering-parameter extractions from 3 He + 4 He ⃗ 7 Be + γ

Journal of physics. G, Nuclear and particle physics, 2020-03, Vol.47 (5)

2020

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Models, measurements, and effective field theory: Proton capture on Be 7 at next-to-leading order

Physical review. C, 2018-09, Vol.98 (3), Article 034616

2018

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Models, measurements, and effective field theory: Proton capture on Be7 at next-to-leading order

Physical review. C, 2018-09, Vol.98 (3)

2018

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THE PRIMORDIAL DEUTERIUM ABUNDANCE OF THE MOST METAL-POOR DAMPED Lyα SYSTEM

The Astrophysical journal, 2016-10, Vol.830 (2), p.148

2016

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THE PRIMORDIAL DEUTERIUM ABUNDANCE OF THE MOST METAL-POOR DAMPED Ly SYSTEM∗ ∗ Based on observations collected at the European Organisation for Astronomical Research in the Southern Hemisphere, Chile (VLT program ID: 093.A-0016(A)), and at the W.M. Keck Observatory which is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financia

The Astrophysical journal, 2016-10, Vol.830 (2)

2016

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How well do we understand 7 Be + p → 8 B + γ ? An Effective Field Theory perspective

EPJ Web of conferences, 2016, Vol.113, p.6001

2016

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How well do we understand 7Be + p → 8B + γ? An Effective Field Theory perspective

EPJ Web of Conferences, 2016, Vol.113, p.06001

2016

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Halo effective field theory constrains the solar 7Be + p → 8B + γ rate

Physics letters. B, 2015-12, Vol.751 (C), p.535-540

2015

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BBN and the CMB constrain neutrino coupled light WIMPs

Physical review. D, Particles, fields, gravitation, and cosmology, 2015-04, Vol.91 (8), Article 083505

2015

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Light WIMPs and Equivalent Neutrinos

Physics procedia, 2015, Vol.61, p.179-187

2015

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Combining ab initio calculations and low-energy effective field theory for halo nuclear systems: The case of Be 7 + p → B 8 + γ

Physical review. C, Nuclear physics, 2014-05, Vol.89 (5), Article 051602

2014

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BBN and the CMB constrain light, electromagnetically coupled WIMPs

Physical review. D, Particles, fields, gravitation, and cosmology, 2014-04, Vol.89 (8), Article 083508

2014

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Combining ab initio calculations and low-energy effective field theory for halo nuclear systems: The case of 7 Li + n → 8 Li + γ

Physical review. C, Nuclear physics, 2014-02, Vol.89 (2), Article 024613

2014

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Ab initio calculations of nuclear widths via an integral relation

Physical review. C, Nuclear physics, 2012-10, Vol.86 (4), Article 044330

Nollett, Kenneth M.

2012

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Asymptotic normalization coefficients from ab initio calculations

Physical review. C, Nuclear physics, 2011-04, Vol.83 (4)

2011

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Asymptotic normalization coefficients from ab initio calculations

Physical review. C, Nuclear physics, 2011-04, Vol.83 (4), Article 041001

2011

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On Possible Variation in the Cosmological Baryon Fraction

The Astrophysical journal, 2010-06, Vol.716 (2), p.907-913

2010

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Can Extra Mixing in RGB and AGB Stars Be Attributed to Magnetic Mechanisms?

The Astrophysical journal, 2007-12, Vol.671 (1), p.802-810

2007

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Quantum Monte Carlo calculations of neutron-alpha scattering

Physical review letters, 2007-07, Vol.99 (2), p.022502-022502, Article 022502

2007

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Quantum Monte Carlo Calculations of Neutron-{alpha} Scattering

Physical review letters, 2007-07, Vol.99 (2)

2007

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Modern theories of low-energy astrophysical reactions

Nuclear physics. A, 2006-10, Vol.777, p.111-136

2006

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Piecewise moments method: Generalized Lanczos technique for nuclear response surfaces

Physical review. C, Nuclear physics, 2005-12, Vol.72 (6), Article 065501

2005

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Variational Monte Carlo calculations of n + H 3 scattering

S -factor and scattering-parameter extractions from ^{3}\mathrm{He}+{}^{4}\mathrm{He}{ \rightarrow }^{7}\mathrm{Be}+\gamma

S-factor and scattering-parameter extractions from 3 He + 4 He ⃗ 7 Be + γ

Models, measurements, and effective field theory: Proton capture on Be 7 at next-to-leading order

Models, measurements, and effective field theory: Proton capture on Be7 at next-to-leading order

THE PRIMORDIAL DEUTERIUM ABUNDANCE OF THE MOST METAL-POOR DAMPED Lyα SYSTEM

How well do we understand 7 Be + p → 8 B + γ ? An Effective Field Theory perspective

How well do we understand 7Be + p → 8B + γ? An Effective Field Theory perspective

Halo effective field theory constrains the solar 7Be + p → 8B + γ rate

BBN and the CMB constrain neutrino coupled light WIMPs

Light WIMPs and Equivalent Neutrinos

Combining ab initio calculations and low-energy effective field theory for halo nuclear systems: The case of Be 7 + p → B 8 + γ

BBN and the CMB constrain light, electromagnetically coupled WIMPs

Combining ab initio calculations and low-energy effective field theory for halo nuclear systems: The case of 7 Li + n → 8 Li + γ

Ab initio calculations of nuclear widths via an integral relation

Asymptotic normalization coefficients from ab initio calculations

Asymptotic normalization coefficients from ab initio calculations

Solar fusion cross sections. II. The p p chain and CNO cycles

On Possible Variation in the Cosmological Baryon Fraction

Can Extra Mixing in RGB and AGB Stars Be Attributed to Magnetic Mechanisms?

Quantum Monte Carlo calculations of neutron-alpha scattering

Quantum Monte Carlo Calculations of Neutron-{alpha} Scattering

Modern theories of low-energy astrophysical reactions

Piecewise moments method: Generalized Lanczos technique for nuclear response surfaces

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