Falk Herwig

0000-0001-8087-9278

astro-ph.SRastro-phastro-ph.HEastro-ph.GAnucl-thnucl-exastro-ph.EPastro-ph.IMphysics.flu-dyngr-qc

On Valency

published · living versions

W_waqfzrqh·v1 · currentpublished

Catching Element Formation In The Act

with Chris L. Fryer, Frank Timmes, Aimee L. Hungerford, Aaron Couture +214

1 version

Preprints & journals

142 papers in the corpus · 1998–2026

The physics of deep-interior convective shell boundaries in a massive pre-supernova star: Internal gravity wave mixing at the

N^2

peak2609.28667v1 · Praneet Pathak, Falk Herwig, Simon Blouin et al.2026 · 0 citationsarXiv

Testing a Pre-Supernova Contribution to

^{44}

Ti in Cassiopeia A2609.16826v1 · Toshiki Sato, Joshua Issa, Falk Herwig et al.2026 · 0 citationsarXiv

Wave-Driven Mixing Enhanced by Rotation in Red Giant Branch Stars2606.30541v1 · Simon Blouin, Paul R. Woodward, Pavel A. Denissenkov et al.2026 · 3 citationsNat Astron 10, 385-390 (2026)

Can COSI detect

\gamma

-ray lines from rare isotopes produced in the astrophysical intermediate neutron-capture process?2605.27829v3 · Falk Herwig, Pavel Denissenkov, Eric Burns2026 · 0 citationsarXiv

Stellar Interpretation of Meteoritic Data and PLotting for Everyone (SIMPLE): Isotope Mixing Lines for Six Sets of Core-Collapse Supernova Models2602.04354v1 · Marco Pignatari, Mattias Ek, Georgy V. Makhatadze et al.2026 · 0 citationsarXiv

The NuGrid AGB Evolution and Nucleosynthesis Data Set2601.05723v1 · Umberto Battino, Marco Pignatari, Ashley Tattersall et al.2026 · 7 citationsUniverse 2022, 8, 170

Propagating Uncertainties from Nuclear Physics to Gamma-rays in Core Collapse Supernovae2601.04464v1 · Chris L Fryer, Hendrik Schatz, Samuel Jones et al.2026 · 0 citationsarXiv

Pre-supernova O-C shell mergers could produce more

^{44}\mathrm{Ti}

than the explosion2512.17705v6 · Joshua Issa, Falk Herwig2025 · 2 citationsarXiv

NoxO1 promotes endosome formation and reduces intracellular vesicle processing.41406574 · Hebchen, Maureen, Herwig, Falk, Schader, Tim et al.2026 · 1 citationRedox biology. 2026;89:103973

Calcium Excess in Novae: Beyond Nuclear Physics Uncertainties2511.04874v1 · Mallory Loria, Pavel Denissenkov, Chris Ruiz et al.2025 · 0 citationsApJ 993 156 (2025)

Production of radioactive

^{22}

Na in core-collapse supernovae: the Ne-E(L) component in presolar grains and its possible consequences on supernova observations2510.16246v1 · M. Pignatari, S. Amari, P. Hoppe et al.2025 · 3 citationsThe Astrophysical Journal, Volume 990, Issue 1, id.19, 10 pp. 2025

3D Macro Physics and Light Odd-Z Element Production in O-C Shell Mergers: Implications for

^{40}\mathrm{K}

production and radiogenic heating inventories of rocky exoplanets2509.19240v2 · Joshua Issa, Falk Herwig, Stephen J. Mojzsis et al.2025 · 5 citationsarXiv

Trans-Fe elements from Type Ia Supernovae. I. Heavy element nucleosynthesis during the formation of near-Chandrasekhar white dwarfs2508.15079v1 · Umberto Battino, James Keegans, Megan Allen et al.2025 · 0 citationsA&A 703, A44 (2025)

3D hydrodynamic simulations of massive main-sequence stars -- IV. Internal gravity waves matter for SLF variability2508.03893v2 · Praneet Pathak, Simon Blouin, Falk Herwig et al.2025 · 1 citationarXiv

Impact of 3D macro physics and nuclear physics on the p nuclei in O-C shell mergers2507.16965v2 · Joshua Issa, Falk Herwig, Pavel Denissenkov et al.2025 · 4 citationsarXiv

Multidisciplinary Science in the Multimessenger Era2502.03577v3 · Eric Burns, Christopher L. Fryer, Ivan Agullo et al.2025 · 1 citationarXiv

Quantifying systematic uncertainties in white dwarf cooling age determinations2410.14014v2 · Praneet Pathak, Simon Blouin, Falk Herwig2024 · 6 citationsarXiv

First Study of the ^139Ba(n,γ)^140Ba Reaction to Constrain the Conditions for the Astrophysical i Process.38829093 · Spyrou, A, Mücher, D, Denissenkov, P A et al.2024 · 13 citationsPhysical review letters. 2024;132(20):202701

Thallium-208: A Beacon of In Situ Neutron Capture Nucleosynthesis.38364162 · Vassh, Nicole, Wang, Xilu, Larivière, Maude et al.2024 · 13 citationsPhysical review letters. 2024;132(5):052701

Enhanced extra mixing in low-mass stars approaching the RGB tip and the problem of Li-rich red-clump stars2309.04634v2 · Pavel A. Denissenkov (UVic), Simon Blouin (UVic), Falk Herwig (UVic) et al.2023 · 9 citationsarXiv

3D hydrodynamics simulations of a 3

M_{\odot}

core-helium burning star2308.10865v2 · Simon Blouin, Falk Herwig, Huaqing Mao et al.2023 · 0 citationsarXiv

3D hydrodynamic simulations of massive main-sequence stars. III. The effect of radiation pressure and diffusion leading to a 1D equilibrium model2304.10470v2 · Huaqing Mao, Paul Woodward, Falk Herwig et al.2023 · 8 citationsarXiv

3D hydrodynamics simulations of core convection in supermassive main-sequence stars2303.10115v1 · Simon Blouin, Huaqing Mao, Tyrone E. Woods et al.2023 · 3 citationsarXiv

3D hydrodynamics simulations of internal gravity waves in red giant branch stars2303.07332v1 · Simon Blouin, Huaqing Mao, Falk Herwig et al.2023 · 20 citationsarXiv

3D hydrodynamic simulations of massive main-sequence stars II. Convective excitation and spectra of internal gravity waves2303.06125v4 · William Thompson, Falk Herwig, Paul R. Woodward et al.2023 · 26 citationsarXiv

3D hydrodynamic simulations of massive main-sequence stars. I. Dynamics and mixing of convection and internal gravity waves2303.05495v3 · Falk Herwig, Paul R. Woodward, Huaqing Mao et al.2023 · 37 citationsarXiv

Measuring neutron capture cross sections of radioactive nuclei: From activations at the FZK Van de Graaff to direct neutron captures in inverse kinematics with a storage ring at TRIUMF.37187510 · Dillmann, Iris, Kester, Oliver, Baartman, Richard et al.2023 · 9 citationsThe European physical journal. A, Hadrons and nuclei. 2023;59(5):105

Modules for Experiments in Stellar Astrophysics (MESA): Time-Dependent Convection, Energy Conservation, Automatic Differentiation, and Infrastructure2208.03651v2 · Adam S. Jermyn, Evan B. Bauer, Josiah Schwab et al.2022 · 604 citationsarXiv

Horizons: Nuclear Astrophysics in the 2020s and Beyond2205.07996v1 · H. Schatz, A. D. Becerril Reyes, A. Best et al.2022 · 51 citationsarXiv

Dynamics in a stellar convective layer and at its boundary: Comparison of five 3D hydrodynamics codes2111.01165v2 · R. Andrassy, J. Higl, H. Mao et al.2021 · 21 citationsA&A 659, A193 (2022)

Study of (

^6

Li,

d

) and (

^6

Li,

t

) reactions on

^{22}

Ne and implications for

s

-process nucleosynthesis2107.00131v1 · S. Ota, G. Christian, W. N. Catford et al.2021 · 18 citationsPhys. Rev. C 104, 055806 (2021)

R Coronae Borealis Star Evolution: Simulating 3D Merger Events to 1D Stellar Evolution Including Large Scale Nucleosynthesis2103.01741v1 · Bradley Munson, Emmanouil Chatzopoulos, Juhan Frank et al.2021 · 20 citationsarXiv

The impact of (n,

\gamma

) reaction rate uncertainties of unstable isotopes on the i-process nucleosynthesis of the elements from Ba to W2010.15798v2 · Pavel A. Denissenkov (UVic), Falk Herwig (UVic), Georgios Perdikakis (CMU) et al.2020 · 27 citationsarXiv

An evidence-based assumption that helps to reduce the discrepancy between the observed and predicted

^7

Be abundances in novae2010.09825v2 · Pavel A. Denissenkov (UVic), Chris Ruiz (TRIUMF), Sriteja Upadhyayula (TRIUMF) et al.2020 · 11 citationsarXiv

Heavy Elements Nucleosynthesis On Accreting White Dwarfs: building seeds for the p-process2007.13677v1 · Umberto Battino, Marco Pignatari, Claudia Travaglio et al.2020 · 20 citationsarXiv

Convective H-He Interactions in Massive Population III Stellar Evolution Models2005.07748v2 · Ondrea Clarkson, Falk Herwig2020 · 53 citationsarXiv

3D1D hydro-nucleosynthesis simulations. I. Advective-reactive post-processing method and its application to H ingestion into He-shell flash convection in rapidly accreting white dwarfs2001.10969v2 · David Stephens (UVic), Falk Herwig (UVic), Paul Woodward (U. of Minnesota) et al.2020 · 24 citationsarXiv

The Impact of Nuclear Physics Uncertainties on Galactic Chemical Evolution Predictions1911.00035v1 · Benoit Cot'e, Pavel Denissenkov, Falk Herwig et al.2019 · 1 citationarXiv

LRP2020: The cosmic origin and evolution of the elements1910.09712v1 · Rodrigo Fern'andez, Falk Herwig, Samar Safi-Harb et al.2019 · 0 citationsarXiv

The impact of (n,

\gamma

) reaction rate uncertainties on the predicted abundances of i-process elements with

32\leq Z\leq 48

in the metal-poor star HD940281909.07011v2 · John E. McKay (UVic, TRIUMF), Pavel A. Denissenkov (UVic) et al.2019 · 18 citationsarXiv

The s process in rotating low-mass AGB stars. Nucleosynthesis calculations in models matching asteroseismic constraints1908.09160v1 · J.W. den Hartogh, R. Hirschi, M. Lugaro et al.2019 · 22 citationsA&A 629, A123 (2019)

Chromium Nucleosynthesis and Silicon-Carbon Shell Mergers in Massive Stars1906.07218v1 · Benoit Cot'e, Samuel Jones, Falk Herwig et al.2019 · 7 citationsarXiv

NuGrid stellar data set - III. Updated low-mass AGB models and s-process nucleosynthesis with metallicities Z=0.01, Z=0.02 and Z=0.031906.01952v1 · Umberto Battino, Ashley Tattersall, Claudia Lederer-Woods et al.2019 · 64 citationsarXiv

Catching Element Formation In The Act1902.02915v1 · Chris L. Fryer, Frank Timmes, Aimee L. Hungerford et al.2019 · 17 citationsarXivon Valency

Nucleosynthetic Yields from Neutron Stars Accreting in Binary Common Envelopes1902.01661v1 · James D. Keegans, Chris L. Fryer, Samuel W. Jones et al.2019 · 8 citationsarXiv

Simulating 3-D Stellar Hydrodynamics using PPM and PPB Multifluid Gas Dynamics on CPU and CPU+GPU Nodes1810.13416v1 · Paul R. Woodward, Pei-Hung Lin, Huaqing Mao et al.2018 · 11 citationsarXiv

H-He Shell Interactions and Nucleosynthesis in Massive Population III Stars1810.12259v1 · Ondrea Clarkson, Falk Herwig, Robert Andrassy et al.2018 · 2 citationsarXiv

The i-process yields of rapidly-accreting white dwarfs from multicycle He-shell flash stellar evolution models with mixing parameterizations from 3D hydrodynamics simulations1809.03666v2 · Pavel Denissenkov (UVic), Falk Herwig (UVic), Paul Woodward (U. of Minnesota) et al.2018 · 84 citationsarXiv

Experimentally well-constrained masses of

^{27}

P and

^{27}

S: Implications for studies of explosive binary systems1809.02980v2 · L. J. Sun, X. X. Xu, S. Q. Hou et al.2018 · 20 citationsarXiv

3D hydrodynamic simulations of C ingestion into a convective O shell1808.04014v2 · Robert Andrassy, Falk Herwig, Paul Woodward et al.2018 · 63 citationsarXiv

Career total: at least 337 works. 142 are in this corpus.Showing the 50 most recent.

Profile built from the corpus for this byline.

337

works

9,363

citations

h-index

Corpus papers per year

Corpus papers per year, 1998 to 2026. Busiest year 2008, 11 papers.
Year	Papers
1998	1
1999	0
2000	0
2001	2
2002	4
2003	1
2004	2
2005	4
2006	7
2007	8
2008	11
2009	1
2010	4
2011	1
2012	7
2013	10
2014	7
2015	4
2016	9
2017	8
2018	6
2019	8
2020	5
2021	3
2022	2
2023	9
2024	2
2025	9
2026	7

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