DiRAC-3 Operations - 2022-23 extension - Cambridge
Lead Research Organisation:
University of Cambridge
Department Name: Institute of Astronomy
Abstract
This grant is a costed 12-month extension of the grant "DiRAC-3 Operations 2019-2022 - Cambridge [2020-06 resubmission]", (STFC reference: ST/V002635/1).
Organisations
Publications
Orkney M
(2023)
Exploring the diversity and similarity of radially anisotropic Milky Way-like stellar haloes: implications for disrupted dwarf galaxy searches
in Monthly Notices of the Royal Astronomical Society
Page B
(2023)
Novel bottomonium results
Pakmor R
(2023)
The MillenniumTNG Project: the hydrodynamical full physics simulation and a first look at its galaxy clusters
in Monthly Notices of the Royal Astronomical Society
Pandya A
(2022)
Dynamics of a nonminimally coupled scalar field in asymptotically AdS 4 spacetime
in Classical and Quantum Gravity
Pariat E
(2023)
Comparison of magnetic energy and helicity in coronal jet simulations
in Astronomy & Astrophysics
Parrott W
(2023)
Standard Model predictions for B ? K l + l - , B ? K l 1 - l 2 + and B ? K ? ? ¯ using form factors from N f = 2 + 1 + 1 lattice QCD
in Physical Review D
Parrott W
(2022)
$V_{cs}$ determination from $D \to{}K \ell \nu$
Parrott W
(2023)
B ? K and D ? K form factors from fully relativistic lattice QCD
in Physical Review D
Pastorek A
(2022)
Time-resolved fourier transform infrared emission spectroscopy of NH radical in the X3S- ground state
in Journal of Quantitative Spectroscopy and Radiative Transfer
Pastorek A
(2022)
New physical insights: Formamide discharge decomposition and the role of fragments in the formation of large biomolecules
in Spectrochimica Acta Part A: Molecular and Biomolecular Spectroscopy
Pellen M
(2022)
Angular coefficients in $$\hbox {W}+\hbox {j}$$ production at the LHC with high precision
in The European Physical Journal C
Pereira-Wilson M
(2023)
The cosmic UV background and the beginning and end of star formation in simulated field dwarf galaxies
in Monthly Notices of the Royal Astronomical Society
Pfeffer J
(2023)
Globular cluster metallicity distributions in the E-MOSAICS simulations
in Monthly Notices of the Royal Astronomical Society
Pfeffer J
(2022)
Using the EAGLE simulations to elucidate the origin of disc surface brightness profile breaks as a function of mass and environment
in Monthly Notices of the Royal Astronomical Society
Pierens A
(2023)
Three-dimensional evolution of radiative circumbinary discs: The size and shape of the inner cavity
in Astronomy & Astrophysics
Ploeckinger S
(2024)
Resolution criteria to avoid artificial clumping in Lagrangian hydrodynamic simulations with a multiphase interstellar medium
in Monthly Notices of the Royal Astronomical Society
Prgomet M
(2022)
EDGE: The sensitivity of ultra-faint dwarfs to a metallicity-dependent initial mass function
in Monthly Notices of the Royal Astronomical Society
Prole L
(2023)
From dark matter halos to pre-stellar cores: high resolution follow-up of cosmological Lyman-Werner simulations
in Monthly Notices of the Royal Astronomical Society
Prole L
(2022)
Primordial magnetic fields in Population III star formation: a magnetized resolution study
in Monthly Notices of the Royal Astronomical Society
Qiao L
(2022)
The evolution of protoplanetary discs in star formation and feedback simulations
in Monthly Notices of the Royal Astronomical Society
Quinn J
(2022)
Flute and kink instabilities in a dynamically twisted flux tube with anisotropic plasma viscosity
in Monthly Notices of the Royal Astronomical Society
RamÃrez-Galeano L
(2022)
Why most molecular clouds are gravitationally dominated
in Monthly Notices of the Royal Astronomical Society
Ratnasingam R
(2023)
Internal gravity waves in massive stars II. Frequency analysis across stellar mass
in Astronomy & Astrophysics