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arXiv 2017年

作者： Morales, José A. E. Gamba, Irene M. Endeve, Eirik Hauck, Cory TU Wien Institute for Analysis and Scientific Computing University of Texas at Austin Institute for Computational Engineering and Sciences Department of Mathematics Oak Ridge National Lab Computational and Applied Mathematics Group

The work presented in this paper is related to the development of positivity preserving Discontinuous Galerkin (DG) methods for Boltzmann - Poisson (BP) computational models of electronic transport in semiconductors. We pose the Boltzmann Equation for electron transport in curvilinear coordinates for the momentum. We consider the 1D diode problem with azimuthal symmetry, which is a 3D plus time problem. We choose for this problem the spherical coordinate system p→(|p→|, μ = cosθ, φ), slightly different to the choice in previous DG solvers for BP, because its DG formulation gives simpler integrals involving just piecewise polynomial functions for both transport and collision terms. Applying the strategy of Zhang & Shu, [1], [2], Cheng, Gamba, Proft, [3], and Endeve et al. [4], we treat the collision operator as a source term, and find convex combinations of the transport and collision terms which guarantee the positivity of the cell average of our numerical probability density function at the next time step. The positivity of the numerical solution to the pdf in the whole domain is guaranteed by applying the limiters in [1], [2] that preserve the cell average but modify the slope of the piecewise linear solutions in order to make the function non - negative. In addition of the proofs of positivity preservation in the DG scheme, we prove the stability of the semi-discrete DG scheme under an entropy norm, using the dissipative properties of our collisional operator given by its entropy inequalities. The entropy inequality we use depends on an exponential of the Hamiltonian rather than the Maxwellian associated just to the kinetic energy. Copyright © 2017, The Authors. All rights reserved.

关键词： Galerkin methods

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A homogenization theorem for langevin systems with an application to hamiltonian dynamics

arXiv

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arXiv 2017年

作者： Birrell, Jeremiah Wehr, Jan Department of Mathematics University of Arizona TucsonAZ85721 United States Department of Mathematics and Program in Applied Mathematics University of Arizona TucsonAZ85721 United States

This paper studies homogenization of stochastic differential systems. The standard example of this phenomenon is the small mass limit of Hamiltonian *** consider this case first from the heuristic point of view, stressing the role of detailed balance and presenting the heuristics based on a multiscale expansion. This is used to propose a physical interpretation of recent results by the authors, as well as to motivate a new theorem proven here. Its main content is a sufficient condition, expressed in terms of solvability of an associated partial differential equation ("the cell problem"), under which the homogenization limit of an SDE is calculated explicitly. The general theorem is applied to a class of systems, satisfying a generalized detailed balance condition with a position-dependent temperature. Copyright © 2017, The Authors. All rights reserved.

关键词： Stochastic systems

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Multireference alignment is easier with an aperiodic translation distribution

arXiv

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arXiv 2017年

作者： Abbe, Emmanuel Bendory, Tamir Leeb, William Pereira, João M. Sharon, Nir Singer, Amit Program in Applied and Computational Mathematics Princeton University PrincetonNJ United States Electrical Engineering Department Princeton University PrincetonNJ United States Department of Mathematics Princeton University PrincetonNJ United States

In the multireference alignment model, a signal is observed by the action of a random circular translation and the addition of Gaussian noise. The goal is to recover the signal's orbit by accessing multiple independent observations. Of particular interest is the sample complexity, i.e., the number of observations/samples needed in terms of the signal-to-noise ratio (the signal energy divided by the noise variance) in order to drive the mean-square error (MSE) to zero. Previous work showed that if the translations are drawn from the uniform distribution, then, in the low SNR regime, the sample complexity of the problem scales as ω(1/SNR3). In this work, using a generalization of the Chapman-Robbins bound for orbits and expansions of the X2divergence at low SNR, we show that in the same regime the sample complexity for any aperiodic translation distribution scales as ω(1/SNR2). This rate is achieved by a simple spectral algorithm. We propose two additional algorithms based on non-convex optimization and expectation-maximization. We also draw a connection between the multireference alignment problem and the spiked covariance model. Copyright © 2017, The Authors. All rights reserved.

关键词： Maximum principle

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Locating and counting equilibria of the Kuramoto model with rank one coupling

arXiv

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arXiv 2017年

作者： Coss, Owen Hauenstein, Jonathan D. Hong, Hoon Molzahn, Daniel K. Department of Mathematics North Carolina State University Department of Applied and Computational Mathematics and Statistics University of Notre Dame Energy Systems Division Argonne National Laboratory

The Kuramoto model describes synchronization behavior among coupled oscillators and enjoys successful application in a wide variety of fields. Many of these applications seek phase-coherent solutions, i.e., equilibria of the model. Historically, research has focused on situations where the number of oscillators, n, is extremely large and can be treated as being infinite. More recently, however, applications have arisen in areas such as electrical engineering with more modest values of n. For these, the equilibria can be located by finding the real solutions of a system of polynomial equations utilizing techniques from algebraic geometry. However, typical methods for solving such systems locate all complex solutions even though only the real solutions give equilibria. In this paper, we present an algorithm to locate only the real solutions of the model, thereby shortening computation time by several orders of magnitude in certain situations. This is accomplished by choosing specific equilibria representatives and the consequent algebraic decoupling of the system. The correctness of the algorithm (that it finds only and all the equilibria) is proved rigorously. Additionally, the algorithm can be implemented using interval methods so that the equilibria can be approximated up to any given precision without significantly more computational effort. We also compare this solving approach to other computational algebraic geometric methods. Furthermore, analyzing this approach allows us to prove, asymptotically, that the maximum number of equilibria grows at the same rate as the number of complex solutions of a corresponding polynomial system. Finally, we conjecture an upper bound on the maximum number of equilibria for any number of oscillators which generalizes the known cases and is obtained on a range of explicitly provided natural *** Codes 65H10, 68W30, 14Q99 Copyright © 2017, The Authors. All rights reserved.

关键词： Geometry

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Extended calculations of energy levels, radiative properties, AJ, BJ hyperfine interaction constants, and Landé gJ-factors for nitrogen-like Ge XXVI

arXiv

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arXiv 2018年

作者： Wang, K. Zhang, C.Y. Jönsson, P. Si, R. Zhao, X.H. Chen, Z.B. Guo, X.L. Chen, C.Y. Yan, J. Hebei Key Lab of Optic-electronic Information and Materials College of Physics Science and Technology Hebei University Baoding071002 China Group for Materials Science and Applied Mathematics Malmö University MalmöSE-20506 Sweden Shanghai EBIT Lab Institute of Modern Physics Department of Nuclear Science and Technology Fudan University Shanghai200433 China School of Science Hunan University of Technology Zhuzhou412007 China Department of Radiotherapy Shanghai Changhai Hospital Shanghai200433 China Institute of Applied Physics and Computational Mathematics Beijing100088 China

Employing two state-of-the-art methods, multiconfiguration Dirac–Hartree–Fock and second-order many-body perturbation theory, highly accurate calculations are performed for the lowest 272 fine-structure levels arising from the 2s22p3, 2s2p4, 2p5, 2s22p23l (l = s, p, d), 2s2p33l (l = s, p, d), and 2p43l (l = s, p, d) configurations in nitrogen-like Ge XXVI. Complete and consistent atomic data, including excitation energies, lifetimes, wavelengths, hyperfine structures, Landé gJ-factors, and E1, E2, M1, M2 line strengths, oscillator strengths, and transition rates among these 272 levels are provided. Comparisons are made between the present two data sets, as well as with other available experimental and theoretical values. The present data are accurate enough for identification and deblending of emission lines involving the n = 3 levels, and are also useful for modeling and diagnosing fusion plasmas. Copyright © 2018, The Authors. All rights reserved.

关键词： Nitrogen

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Partial deconfinement at strong coupling on the lattice

arXiv

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arXiv 2020年

作者： Watanabe, Hiromasa Bergner, Georg Bodendorfer, Norbert Funai, Shotaro Shiba Hanada, Masanori Rinaldi, Enrico Schäfer, Andreas Vranas, Pavlos Graduate School of Pure and Applied Sciences University of Tsukuba Tsukuba Ibaraki305-8571 Japan University of Jena Institute for Theoretical Physics Max-Wien-Platz 1 JenaD-07743 Germany University of Regensburg Institute of Theoretical Physics Universitätsstrasse 31 D-93053 Germany 1919-1 Tancha Onna-son Kunigami-gun Okinawa904-0495 Japan Department of Mathematics University of Surrey Guildford SurreyGU2 7XH United Kingdom Arithmer Inc. R&D Headquarters Minato Tokyo106-6040 Japan RIKEN iTHEMS Program Wako Saitama351-0198 Japan Nuclear and Chemical Sciences Division Lawrence Livermore National Laboratory LivermoreCA94550 United States Nuclear Science Division Lawrence Berkeley National Laboratory BerkeleyCA94720 United States

We provide evidence for partial deconfinement - the deconfinement of a SU(M) subgroup of the SU(N) gauge group - by using lattice Monte Carlo simulations. We take matrix models as concrete examples. By appropriately fixing the gauge, we observe that the M×M submatrices deconfine. This gives direct evidence for partial deconfinement at strong coupling. We discuss the applications to QCD and holography. Copyright © 2020, The Authors. All rights reserved.

关键词： Monte Carlo methods

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The NuSTAR Serendipitous Survey: the 80-month catalog and source properties of the high-energy emitting AGN and quasar population

arXiv

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arXiv 2024年

作者： Greenwell, Claire L. Klindt, Lizelke Lansbury, George B. Rosario, David J. Alexander, David M. Aird, James Stern, Daniel Forster, Karl Koss, Michael J. Bauer, Franz E. Ricci, Claudio Tomsick, John Brandt, William N. Connor, Thomas Boorman, Peter G. Annuar, Adlyka Ballantyne, David R. Chen, Chien-Ting Civano, Francesca Comastri, Andrea Fawcett, Victoria A. Fornasini, Francesca M. Gandhi, Poshak Harrison, Fiona Heida, Marianne Hickox, Ryan Kammoun, Elias S. Lanz, Lauranne Marchesi, Stefano Noirot, Gaël Romero-Colmenero, Encarni Treister, Ezequiel Urry, C. Megan Väisänen, Petri van Soelen, Brian Centre for Extragalactic Astronomy Department of Physics Durham University DurhamDH1 3LE United Kingdom European Southern Observatory Karl-Schwarzschild str. 2 Garching bei MünchenD-85748 Germany School of Mathematics Statistics and Physics Newcastle University Herschel Building Newcastle upon TyneNE1 7RU United Kingdom Institute for Astronomy University of Edinburgh Royal Observatory EdinburghEH9 3HJ United Kingdom School of Physics & Astronomy University of Leicester University Road LeicesterLE1 7RJ United Kingdom Jet Propulsion Laboratory California Institute of Technology 4800 Oak Grove Drive Mail Stop 169-221 PasadenaCA91109 United States Cahill Center for Astrophysics California Institute of Technology 1216 East California Boulevard PasadenaCA91125 United States Eureka Scientific 2452 Delmer Street Suite 100 OaklandCA94602-3017 United States Space Science Institute 4750 Walnut Street Suite 205 BoulderCO80301 United States Instituto de Astrofísica Centro de Astroingeniería Facultad de Física Pontificia Universidad Católica de Chile Casilla 306 Santiago22 Chile Millennium Institute of Astrophysics Nuncio Monseñor Sótero Sanz 100 Of 104 Providencia Santiago Chile Instituto de Estudios Astrofísicos Facultad de Ingeniería y Ciencias Universidad Diego Portales Av. Ejército Libertador 441 Santiago Chile Kavli Institute for Astronomy and Astrophysics Peking University Beijing100871 China Space Sciences Laboratory University of California 7 Gauss Way BerkeleyCA94720-7450 United States Department of Astronomy and Astrophysics The Pennsylvania State University 525 Davey Lab University ParkPA16802 United States Institute for Gravitation and the Cosmos The Pennsylvania State University University ParkPA16802 United States Department of Physics The Pennsylvania State University University ParkPA16802 United States Astronomical Institute Academy of Sciences Boční’ II 1401 PragueCZ-14131 Czech Republic Department of Applied Ph

We present a catalog of hard X-ray serendipitous sources detected in the first 80 months of observations by the Nuclear Spectroscopic Telescope Array (NuSTAR). The NuSTAR serendipitous survey 80-month (NSS80) catalog has an unprecedented ∼ 62 Ms of effective exposure time over 894 unique fields (a factor of three increase over the 40-month catalog), with an areal coverage of ∼ 36 deg2, larger than all NuSTAR extragalactic surveys. NSS80 provides 1274 hard X-ray sources in the 3 − 24 keV band (822 new detections compared to the previous 40-month catalog). Approximately 76% of the NuSTAR sources have lower-energy (10−40 keV〉 = 1.2 × 1044 erg s−1 and 〈z〉 = 0.56. We investigate the optical properties and construct composite optical spectra to search for subtle signatures not present in the individual spectra, finding an excess of redder BL AGN compared to optical quasar surveys predominantly due to the presence of the host-galaxy and, at least in part, due to dust obscuration. © 2024, CC BY.

关键词： Active Galactic Nuclei

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The observational uncertainty of coronal hole boundaries in automated detection schemes

arXiv

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arXiv 2021年

作者： Reiss, Martin A. Muglach, Karin Möstl, Christian Arge, Charles N. Bailey, Rachel Delouille, Véronique Garton, Tadhg M. Hamada, Amr Hofmeister, Stefan Illarionov, Egor Jarolim, Robert Kirk, Michael S.F. Kosovichev, Alexander Krista, Larisza Lee, Sangwoo Lowder, Chris MacNeice, Peter J. Veronig, Astrid Space Research Institute Austrian Academy of Sciences Graz Austria Heliophysics Science Division NASA Goddard Space Flight Center GreenbeltMD20771 United States Catholic University of America WashingtonDC20064 United States Conrad Observatory Zentralanstalt für Meteorologie und Geodynamik Vienna Austria Royal Observatory of Belgium Brussels Belgium University of Southampton Southampton United Kingdom Space Physics and Astronomy Research Unit Space Climate Group University of Oulu Oulu Finland University of Graz Institute of Physics Graz Austria Columbia Astrophysics Laboratory Columbia University New YorkNY10027 United States Moscow State University Moscow119991 Russia Moscow Center of Fundamental and Applied Mathematics Moscow119234 Russia ASTRA llc LouisvilleCO80027 United States Center for Computational Heliophysics New Jersey Institute of Technology NewarkNJ07102 United States Department of Physics New Jersey Institute of Technology NewarkNJ07102 United States NASA Ames Research Center Moffett FieldCA94035 United States Cooperative Institute for Research in Environmental Sciences University of Colorado BoulderCO80309 United States National Centers for Environmental Information National Oceanic and Atmospheric Administration BoulderCO80305 United States Korean Space Weather Center Jeju Korea Republic of Southwest Research Institute BoulderCO United States Kanzelhöhe Observatory for Solar and Environmental Research University of Graz Graz Austria

Coronal holes are the observational manifestation of the solar magnetic field open to the heliosphere and are of pivotal importance for our understanding of the origin and acceleration of the solar wind. Observations from space missions such as the Solar Dynamics Observatory now allow us to study coronal holes in unprecedented detail. Instrumental effects and other factors, however, pose a challenge to automatically detect coronal holes in solar imagery. The science community addresses these challenges with different detection schemes. Until now, little attention has been paid to assessing the disagreement between these schemes. In this COSPAR ISWAT initiative, we present a comparison of nine automated detection schemes widely-applied in solar and space science. We study, specifically, a prevailing coronal hole observed by the Atmospheric Imaging Assembly instrument on 2018 May 30. Our results indicate that the choice of detection scheme has a significant effect on the location of the coronal hole boundary. Physical properties in coronal holes such as the area, mean intensity, and mean magnetic field strength vary by a factor of up to 4.5 between the maximum and minimum values. We conclude that our findings are relevant for coronal hole research from the past decade, and are therefore of interest to the solar and space research community. © 2021, CC BY.

关键词： Space research

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Thermal generation, manipulation and detection of skyrmions

arXiv

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arXiv 2020年

作者： Wang, Zidong Guo, Minghua Zhou, Heng-An Zhao, Le Xu, Teng Tomasello, Riccardo Bai, Hao Dong, Yiqing Je, Soong Geun Chao, Weilun Han, Hee-Sung Lee, Suseok Lee, Ki-Suk Yao, Yunyan Han, Wei Song, Cheng Wu, Huaqiang Carpentieri, Mario Finocchio, Giovanni Im, Mi-Young Lin, Shi-Zeng Jiang, Wanjun State Key Laboratory of Low-Dimensional Quantum Physics Department of Physics Tsinghua University Beijing100084 China Frontier Science Center for Quantum Information Tsinghua University Beijing100084 China Institute of Microelectronics Tsinghua University Beijing100084 China Institute of Applied and Computational Mathematics FORTH Heraklion-CreteGR-70013 Greece Center for X-ray Optics Advanced Light Source Lawrence Berkeley National Laboratory Cyclotron Road BerkeleyCA94720 United States Department of Physics Chonnam National University Gwangju61186 Korea Republic of School of Materials Science and Engineering Ulsan National Institute of Science and Technology Ulsan44919 Korea Republic of Daegu Gyeongbuk Institute of Science and Technology Daegu711-873 Korea Republic of International Center for Quantum Materials School of Physics Peking University Beijing100871 China School of Materials Science and Engineering Tsinghua University Beijing100084 China Department of Electrical and Information Engineering Polytechnic of Bari Bari70125 Italy Department of Mathematical and Computer Sciences Physical Sciences and Earth Sciences University of Messina Messina98166 Italy Theoretical Division T-4 and CNLS Los Alamos National Laboratory Los AlamosNM87545 United States

Recent years have witnessed significant progresses in realizing skyrmions in chiral magnets1-4 and asymmetric magnetic multilayers5-13, as well as their electrical manipulation2,7,8,10. Equally important, thermal generation, manipulation and detection of skyrmions can be exploited for prototypical new architecture with integrated computation14 and energy harvesting15. It has yet to verify if skyrmions can be purely generated by heating16,17, and if their resultant direction of motion driven by temperature gradients follows the diffusion or, oppositely, the magnonic spin torque17-21. Here, we address these important issues in microstructured devices made of multilayers - [Ta/CoFeB/MgO]15, [Pt/CoFeB/MgO/Ta]15 and [Pt/Co/Ta]15 integrated with on-chip heaters, by using a full-field soft X-ray microscopy. The thermal generation of densely packed skyrmions is attributed to the low energy barrier at the device edge, together with the thermally induced morphological transition from stripe domains to skyrmions. The unidirectional diffusion of skyrmions from the hot region towards the cold region is experimentally observed. It can be theoretically explained by the combined contribution from repulsive forces between skyrmions, and thermal spin-orbit torques in competing with magnonic spin torques17,18,20,21 and entropic forces22. These thermally generated skyrmions can be further electrically detected by measuring the accompanied anomalous Nernst voltages23. The on-chip thermoelectric generation, manipulation and detection of skyrmions could open another exciting avenue for enabling skyrmionics, and promote interdisciplinary studies among spin caloritronics15, magnonics24 and skyrmionics3,4,12. Copyright © 2020, The Authors. All rights reserved.

关键词： Energy harvesting

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The European Reference Genome Atlas: piloting a decentralised approach to equitable biodiversity genomics

NPJ Biodiversity

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NPJ Biodiversity 2024年第1期3卷 28页

作者： Mc Cartney, Ann M. Formenti, Giulio Mouton, Alice De Panis, Diego Marins, Luísa S. Leitão, Henrique G. Diedericks, Genevieve Kirangwa, Joseph Morselli, Marco Salces-Ortiz, Judit Escudero, Nuria Iannucci, Alessio Natali, Chiara Svardal, Hannes Fernández, Rosa De Pooter, Tim Joris, Geert Strazisar, Mojca Wood, Jonathan M. D. Herron, Katie E. Seehausen, Ole Watts, Phillip C. Shaw, Felix Davey, Robert P. Minotto, Alice Fernández, José M. Böhne, Astrid Alegria, Carla Alioto, Tyler Alves, Paulo C. Amorim, Isabel R. Aury, Jean-Marc Backstrom, Niclas Baldrian, Petr Baltrunaite, Laima Barta, Endre Bedhom, Bertrand Belser, Caroline Bergsten, Johannes Bertrand, Laurie Bilandija, Helena Binzer-Panchal, Mahesh Bista, Iliana Blaxter, Mark Borges, Paulo A. V. Dias, Guilherme Borges Bosse, Mirte Brown, Tom Bruggmann, Rémy Buena-Atienza, Elena Burgin, Josephine Buzan, Elena Cariani, Alessia Casadei, Nicolas Chiara, Matteo Chozas, Sergio Jr, Fedor Čiampor Crottini, Angelica Cruaud, Corinne Cruz, Fernando Dalen, Love Biase, Alessiode Delcampo, Javier Delic, Teo Dennis, Aliceb. Derks, Martijn F. L. Diroma, Maria Angela Djan, Mihajla Duprat, Simone Eleftheriadi, Klara Feulner, Philine G. D. Flot, Jean-François Forni, Giobbe Fosso, Bruno Fournier, Pascal Fournier-Chambrillon, Christine Gabaldon, Toni Garg, Shilpa Gissi, Carmela Giupponi, Luca Gomez-Garrido, Jessica González, Josefa Grilo, Miguel L. Grüning, Björn Guerin, Thomas Guiglielmoni, Nadege Gut, Marta Haesler, Marcel P. Hahn, Christoph Halpern, Balint Harrison, Peter W. Heintz, Julia Hindrikson, Maris Höglund, Jacob Howe, Kerstin Hughes, Graham M. Istace, Benjamin Cock, Mark J. Janžekovič, Franc Jonsson, Zophonias O. Joye-Dind, Sagane Koskimäki, Janne J. Krystufek, Boris Kubacka, Justyna Kuhl, Heiner Kusza, Szilvia Labadie, Karine Lähteenaro, Meri Lantz, Henrik Lavrinienko, Anton Leclère, Lucas Lopes, Ricardo Jorge Madsen, Ole Magdelenat, Ghislaine Magoga, Giulia Manousaki, Tereza Mappes, Tapio Marques, Joao Pedro Redondo, Gemma I. Martinez Maumus, Florian McCarthy, Shane A. M Genomics Institute University of California SantaCruz CA United States TheVertebrate Genome Laboratory The Rockefeller University NewYork NY United States Department of Biology University of Florence Sesto Fiorentino Italy InBios-Conservation Genetics Laboratory University of Liege Liege Belgium Leibniz Institut für Zoo und Wildtierforschung Berlin Germany Berlin Center for Genomics in Biodiversity Research Berlin Germany Department of Biology University of Antwerp Antwerp Belgium Institute of Zoology University of Cologne Cologne Germany Department of Chemistry Life Sciences and Environmental Sustainability University of Parma Parma Italy Institute of Evolutionary Biology (CSIC-Universitat Pompeu Fabra Barcelona Spain Naturalis Biodiversity Center Leiden Netherlands Neuromics Support Facility VIB Center for Molecular Neurology VIB Antwerp Belgium Neuromics Support Facility Department of Biomedical SciencesUniversity ofAntwerp Antwerp Belgium Tree of Life WellcomeSanger Institute Cambridge Hinxton United Kingdom School of Biology and Environmental Science University College Dublin Belfield Ireland Aquatic Ecology & Evolution Institute of Ecology & Evolution University of Bern Bern Switzerland Department of Fish Ecology & Evolution Eawag Kastanienbaum Switzerland Department of Biological and Environmental Science University of Jyvaskyla Jyvaskyla Finland The EarlhamInstitute NorwichResearchPark Norwich United Kingdom Digital Science London United Kingdom Barcelona Supercomputing Center Spanish National Bioinformatics Institute ELIXIR Spain Getafe Spain Leibniz Institute for the Analysis of Biodiversity Change Museum Koenig Bonn Bonn Germany CE3C—Centre for Ecology Evolution and Environmental Changes & CHANGE—Global Change and Sustainability Institute Faculdade de Ciências Universidade de Lisboa Campo Grande Lisboa Portugal Centro Nacional de Análisis Genómico (CNAG) Barcelona Spain Universitat de Barcelona (UB) Barcelona Spain CIBIO Cen

A genomic database of all Earth’s eukaryotic species could contribute to many scientific discoveries;however, only a tiny fraction of species have genomic information available. In 2018, scientists across the world united under the Earth BioGenome Project (EBP), aiming to produce a database of highquality reference genomes containing all ~1.5 million recognized eukaryotic species. As the European node of the EBP, the European Reference Genome Atlas (ERGA) sought to implement a new decentralised, equitable and inclusive model for producing reference genomes. For this, ERGA launched a Pilot Project establishing the first distributed reference genome production infrastructure and testing it on 98 eukaryotic species from 33 European countries. Here we outline the infrastructure and explore its effectiveness for scaling high-quality reference genome production, whilst considering equity and inclusion. The outcomes and lessons learned provide a solid foundation for ERGA while offering key learnings to other transnational, national genomic resource projects and the EBP. © The Author(s) 2024, corrected publication 2024.

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