James P Kneller

Neutrino fast flavor oscillations with moments: Linear stability analysis and application to neutron star mergers

PHYSICAL REVIEW D, 109(4).

The SNEWS 2.0 alert software for the coincident detection of neutrinos from core-collapse supernovae

JOURNAL OF INSTRUMENTATION, 19(10).

Two-moment Neutrino Flavor Transformation with Applications to the Fast Flavor Instability in Neutron Star Mergers

ASTROPHYSICAL JOURNAL, 963(1).

Fundamental Symmetries, Neutrons, and Neutrinos (FSNN): Whitepaper for the 2023 NSAC Long Range Plan

Neutrino fast flavor instability in three dimensions for a neutron star merger

PHYSICS LETTERS B, 846.

Advancing the landscape of multimessenger science in the next decade

(2022, March 22). https://arxiv.org/abs/2203.10074

Collaborative experience between scientific software projects using Agile Scrum development

Baxter, A. L., BenZvi, S. Y., Bonivento, W., Brazier, A., Clark, M., Coleiro, A., … Xu, Y. (2022, July 27). SOFTWARE-PRACTICE & EXPERIENCE, Vol. 7.

Neutrino flavor mixing with moments

PHYSICAL REVIEW D, 105(12).

SNEWPY: A Data Pipeline from Supernova Simulations to Neutrino Signals

ASTROPHYSICAL JOURNAL, 925(2).

SNEWS 2.0: a next-generation supernova early warning system for multi-messenger astronomy

[Review of ]. NEW JOURNAL OF PHYSICS, 23(3).

Coupling neutrino oscillations and simulations of core-collapse supernovae

PHYSICAL REVIEW D, 102(8).

IsotropicSQA

(2019, February 21). Zenodo.

IsotropicSQA

(2019, February 21). Zenodo.

IsotropicSQA

(2019, February 21). Zenodo.

Neutrino Quantum Kinetics in Compact Objects

Zenodo.

Neutrino Quantum Kinetics in Compact Objects

Zenodo.

Neutrino Quantum Kinetics in Compact Objects

Zenodo.

Neutrino quantum kinetics in compact objects

PHYSICAL REVIEW D, 99(12).

Neutrinos from Pair Instability Supernovae

Springer Proceedings in Physics, 219, 151–155.

Feasibility of using neutrino intensity interferometry to measure protoneutron star radii

PHYSICAL REVIEW D, 98(4).

Neutrino flavor transformation in supernova as a probe for nonstandard neutrino-scalar interactions

Proceedings of Science, 341. http://www.scopus.com/inward/record.url?eid=2-s2.0-85079340911&partnerID=MN8TOARS

Neutrino flavor transformation in supernovae as a probe for nonstandard neutrino-scalar interactions

PHYSICAL REVIEW D, 97(10).

Neutrino flavour evolution through fluctuating matter

JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS, 45(4).

What can be learned from a future supernova neutrino detection?

Journal of Physics G: Nuclear and Particle Physics, 45(4).

What can be learned from a future supernova neutrino detection?

[Review of ]. Journal of Physics. G, Nuclear and Particle Physics, 45(4).

GR effects in supernova neutrino flavor transformations

PHYSICAL REVIEW D, 96(2).

Neutrino Intensity Interferometry: Measuring Protoneutron Star Radii During Core-Collapse Supernovae

PHYSICAL REVIEW LETTERS, 119(5).

Neutrino signal from pair-instability supernovae

PHYSICAL REVIEW D, 96(10).

Neutrinos from type Ia supernovae: The gravitationally confined detonation scenario

PHYSICAL REVIEW D, 95(4).

The effect of core-collapse supernova accretion phase turbulence on neutrino flavor evolution

Journal of Physics G: Nuclear and Particle Physics, 44(8).

The effect of core-collapse supernova accretion phase turbulence on neutrino flavor evolution

Journal of Physics. G, Nuclear and Particle Physics, 44(8).

Neutrinos from type Ia supernovae: The deflagration-to-detonation transition scenario

PHYSICAL REVIEW D, 94(2).

Nonstandard neutrino interactions in supernovae

PHYSICAL REVIEW D, 94(9).

Supernova Physics at DUNE

(2016, August 28).

The Neutrino: A Better Understanding Through Astrophysics: Final Report

Neutrino Oscillation Above a Black Hole Accretion Disk

NUINT12: 8TH INTERNATIONAL WORKSHOP ON NEUTRINO-NUCLEUS INTERACTIONS IN THE FEW-GEV REGION, Vol. 1663.

Neutrino flavor evolution in turbulent supernova matter

13TH INTERNATIONAL CONFERENCE ON TOPICS IN ASTROPARTICLE AND UNDERGROUND PHYSICS, TAUP 2013, Vol. 61, pp. 729–736.

Sensitivity of neutrinos to the supernova turbulence power spectrum: Point source statistics

PHYSICAL REVIEW D, 92(1).

Stimulated neutrino transformation through turbulence on a changing density profile and application to supernovae

PHYSICAL REVIEW D, 91(2).

The Physics Of Supernova Neutrino Oscillations

(2015, July 6).

Flavor evolution of supernova neutrinos in turbulent matter

1604, 225–232.

Stimulated neutrino transformation through turbulence

PHYSICAL REVIEW D, 89(7).

Turbulence and its effects upon neutrinos

WORKSHOP ON DARK MATTER, NEUTRINO PHYSICS AND ASTROPHYSICS CETUP 2013: VIITH INTERNATIONAL CONFERENCE ON INTERCONNECTIONS BETWEEN PARTICLE PHYSICS AND COSMOLOGY PPC 2013, Vol. 1604, pp. 204–209.

Combining collective, MSW, and turbulence effects in supernova neutrino flavor evolution

PHYSICAL REVIEW D, 88(2).

Consequences of large theta(13) for the turbulence signatures in supernova neutrinos

PHYSICAL REVIEW D, 88(2).

Does the finite size of the proto-neutron star preclude supernova neutrino flavor scintillation due to turbulence?

PHYSICAL REVIEW D, 88(4).

Stimulated neutrino transformation in supernovae

11TH CONFERENCE ON THE INTERSECTIONS OF PARTICLE AND NUCLEAR PHYSICS (CIPANP 2012), Vol. 1560, pp. 176–178.

Stimulated neutrino transformation with sinusoidal density profiles

JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS, 40(5).

v propagation in turbulent supernova matter

11th conference on the intersections of particle and nuclear physics (cipanp 2012), 1560, 333–335.

vs and nucleosynthesis from accretion disks

11TH CONFERENCE ON THE INTERSECTIONS OF PARTICLE AND NUCLEAR PHYSICS (CIPANP 2012), Vol. 1560, pp. 336–340.

ν propagation in turbulent supernova matter

1560, 333–335.

Fundamental Physics at the Intensity Frontier

(2012, May 11).

Neutrino oscillations above black hole accretion disks: Disks with electron-flavor emission

PHYSICAL REVIEW D, 86(8).

The neutrino–neutrino interaction effects in supernovae: the point of view from the ‘matter’ basis

Journal of Physics G: Nuclear and Particle Physics, 39(3).

The 2010 Interim Report of the Long-Baseline Neutrino Experiment Collaboration Physics Working Groups

(2011, October 27).

The effect of turbulence upon supernova neutrinos

Nuclear Physics B - Proceedings Supplements, 217(1), 118–120.

The effect of turbulence upon supernova neutrinos

Nuclear Physics. B, Proceedings, Supplements, 217, 118–120.

Turbulence and supernova neutrinos

Proceedings of the Hamburg Neutrinos from Supernova Explosions, HAvSE 2011, 84–89.

Shock waves in supernovae: New implications on the diffuse supernova neutrino background

Physical Review D, 81(5).

Turbulence effects on supernova neutrinos

Physical Review D, 82(12).

Dynamical Collective Calculation of Supernova Neutrino Signals

PHYSICAL REVIEW LETTERS, 103(7).

Neutrino flavour transformation in supernovae

Journal of Physics G: Nuclear and Particle Physics, 36(11).

Three flavor neutrino oscillations in matter: Flavor diagonal potentials, the adiabatic basis, and the CP phase

PHYSICAL REVIEW D, 80(5).

Oscillation effects and time variation of the supernova neutrino signal

PHYSICAL REVIEW D, 77(4).

Monte Carlo neutrino oscillations

PHYSICAL REVIEW D, 73(5).

Neutrino scattering, absorption and annihilation above the accretion discs of gamma ray bursts

JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS, 32(4), 443–462.

Measuring the amount of dark radiation with the CMB and BBN

Kneller, J. P. (2005, January). NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS, Vol. 138, pp. 73–75.

BBN for pedestrians

New Journal of Physics, 6(2004), 1–22.

BBN for pedestrians

Effect of bound dineutrons upon big bang nucleosynthesis

PHYSICAL REVIEW D, 70(4).

Big bang nucleosynthesis and CMB constraints on dark energy

Physical Review D, 67(6), 063501–063501.

Big bang nucleosynthesis and CMB constraints on dark energy

Physical Review. D, Particles and Fields, 67(6), 063501–063501.

Big bang nucleosynthesis and Lambda(QCD)

PHYSICAL REVIEW D, 68(10).

Effective number of neutrinos and baryon asymmetry from BBN and WMAP

Physics Letters B, 566(1-2), 8–18.

Effective number of neutrinos and baryon asymmetry from BBN and WMAP

Physics Letters. B, 566(02-Jan), 18-.

Hiding relativistic degrees of freedom in the early universe

PHYSICS LETTERS B, 569(3-4), 123–128.

Inverse power law quintessence with nontracking initial conditions

PHYSICAL REVIEW D, 68(8).

Testing Two Nuclear Physics Approximations Used in the Standard Leaky‐Box Model for the Spallogenic Production of LiBeB

The Astrophysical Journal, 589(1 I), 217–224.

CMB (and other) challenges to BBN

Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias, 12, 265–271. http://www.scopus.com/inward/record.url?eid=2-s2.0-0347377313&partnerID=MN8TOARS

How does the cosmic microwave background plus big bang nucleosynthesis constrain new physics?

Physical Review D, 64(12), 6.

How does the cosmic microwave background plus big bang nucleosynthesis constrain new physics?

Physical Review D, 64(12). http://www.scopus.com/inward/record.url?eid=2-s2.0-0035893714&partnerID=MN8TOARS