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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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Big Bang Nucleosynthesis Predictions for Precision Cosmology

The Astrophysical journal, 2001-05, Vol.552 (1), p.L1-L5

2001

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Cool Bottom Processes on the Thermally Pulsing Asymptotic Giant Branch and the Isotopic Composition of Circumstellar Dust Grains

The Astrophysical journal, 2003-01, Vol.582 (2), p.1036-1058

2003

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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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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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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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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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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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On Possible Variation in the Cosmological Baryon Fraction

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

2010

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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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Variational Monte Carlo calculations of n + H 3 scattering

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

2023

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Sharpening the Predictions of Big-Bang Nucleosynthesis

Physical review letters, 1999-05, Vol.82 (21), p.4176-4179

1999

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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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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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Did Very Massive Stars Preenrich and Reionize the Universe?

The Astrophysical journal, 2001-11, Vol.562 (1), p.L1-L4

2001

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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 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 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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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), Article 041001

2011

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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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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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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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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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Estimating reaction rates and uncertainties for primordial nucleosynthesis

Physical review. D, Particles and fields, 2000-06, Vol.61 (12), Article 123505

2000

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

Big Bang Nucleosynthesis Predictions for Precision Cosmology

Cool Bottom Processes on the Thermally Pulsing Asymptotic Giant Branch and the Isotopic Composition of Circumstellar Dust Grains

BBN and the CMB constrain neutrino coupled light WIMPs

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

BBN and the CMB constrain light, electromagnetically coupled WIMPs

Quantum Monte Carlo calculations of neutron-alpha scattering

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

On Possible Variation in the Cosmological Baryon Fraction

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

Variational Monte Carlo calculations of n + H 3 scattering

Sharpening the Predictions of Big-Bang Nucleosynthesis

Modern theories of low-energy astrophysical reactions

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

Did Very Massive Stars Preenrich and Reionize the Universe?

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

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

Ab initio calculations of nuclear widths via an integral relation

Asymptotic normalization coefficients from ab initio calculations

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

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

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

Piecewise moments method: Generalized Lanczos technique for nuclear response surfaces

Estimating reaction rates and uncertainties for primordial nucleosynthesis

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