DiRAC-3 Operations 2023-26 - Durham

Lead Research Organisation: Durham University
Department Name: Physics

Abstract

Abstracts are not currently available in GtR for all funded research. This is normally because the abstract was not required at the time of proposal submission, but may be because it included sensitive information such as personal details.

Publications

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Ali A (2023) Star cluster formation and feedback in different environments of a Milky Way-like galaxy in Monthly Notices of the Royal Astronomical Society

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Altamura E (2023) EAGLE-like simulation models do not solve the entropy core problem in groups and clusters of galaxies in Monthly Notices of the Royal Astronomical Society

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Altamura E (2023) Galaxy cluster rotation revealed in the MACSIS simulations with the kinetic Sunyaev-Zeldovich effect in Monthly Notices of the Royal Astronomical Society

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Alvarez M (2023) NNLO QCD corrections to event shapes at the LHC in Journal of High Energy Physics

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Ananyev V (2023) Collider constraints on electroweakinos in the presence of a light gravitino in The European Physical Journal C

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Appleby S (2023) The physical nature of circumgalactic medium absorbers in Simba in Monthly Notices of the Royal Astronomical Society

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Appleby S (2023) Mapping circumgalactic medium observations to theory using machine learning in Monthly Notices of the Royal Astronomical Society

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Barone A (2023) Approaches to inclusive semileptonic B(s)-meson decays from Lattice QCD in Journal of High Energy Physics

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Barrera M (2023) The MillenniumTNG Project: semi-analytic galaxy formation models on the past lightcone in Monthly Notices of the Royal Astronomical Society

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Bartlett D (2023) Marginalised Normal Regression: Unbiased curve fitting in the presence of x-errors in The Open Journal of Astrophysics

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Bartlett D (2024) Exhaustive Symbolic Regression in IEEE Transactions on Evolutionary Computation

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Bate M (2023) The statistical properties of stars at redshift, z  = 5, compared with the present epoch in Monthly Notices of the Royal Astronomical Society

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Belokurov V (2023) Energy wrinkles and phase-space folds of the last major merger in Monthly Notices of the Royal Astronomical Society

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Bennett E (2024) Singlets in gauge theories with fundamental matter in Physical Review D

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Beraldo E Silva L (2023) Orbital Support and Evolution of Flat Profiles of Bars (Shoulders) in The Astrophysical Journal

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Betts J (2023) Machine learning and structure formation in modified gravity in Monthly Notices of the Royal Astronomical Society

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Borrow J (2023) The impact of stochastic modelling on the predictive power of galaxy formation simulations in Monthly Notices of the Royal Astronomical Society

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Bose S (2023) The MillenniumTNG Project: the large-scale clustering of galaxies in Monthly Notices of the Royal Astronomical Society

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Bose S (2023) The progenitor galaxies of stellar haloes as 'failed' Milky Ways in Monthly Notices of the Royal Astronomical Society

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Braspenning J (2023) Sensitivity of non-radiative cloud-wind interactions to the hydrodynamic solver in Monthly Notices of the Royal Astronomical Society

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Brooks R (2023) The north-south asymmetry of the ALFALFA H i velocity width function in Monthly Notices of the Royal Astronomical Society

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Cardoso V (2023) Curvature and dynamical spacetimes: can we peer into the quantum regime? in Classical and Quantum Gravity

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Chaikin E (2023) A thermal-kinetic subgrid model for supernova feedback in simulations of galaxy formation in Monthly Notices of the Royal Astronomical Society

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Changeat Q (2024) Is the Atmosphere of the Ultra-hot Jupiter WASP-121 b Variable? in The Astrophysical Journal Supplement Series

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Chen C (2023) Can a binary star host three giant circumbinary planets? in Monthly Notices of the Royal Astronomical Society

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Collins C (2023) 3D radiative transfer kilonova modelling for binary neutron star merger simulations in Monthly Notices of the Royal Astronomical Society

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Collins C (2023) Helium as a signature of the double detonation in Type Ia supernovae in Monthly Notices of the Royal Astronomical Society