collaborators

7 papers

gr-qc2026

Bessel-Hagen currents for linearised Weyl-squared gravity

Michael Hobson, Will Barker, Anthony Lasenby

For the Fierz-Pauli action the Bessel-Hagen construction does not produce a preferred local gauge-invariant energy-momentum tensor; it identifies only a gauge-invariant equivalence…

astro-ph.CO2026

Numerical polology: towards next-generation model-building for cosmology

Will Barker, Will Handley, Michael Hobson +4

The dark sector need not be restricted to simple field content. Indeed, simple bosonic configurations, such as scalar-tensor or dark photon models, contrast with the much richer pi…

gr-qc2026

Bessel-Hagen currents for the Fierz-Pauli action

Michael Hobson, Will Barker, Anthony Lasenby

For electromagnetism in Minkowski spacetime, the Bessel-Hagen method gives a particularly direct Noetherian derivation of the standard gauge-invariant energy-momentum tensor. The k…

astro-ph.CO2026

Tilting the scales: weighing prior dependency and global tensions of CMB lensing

A. N. Ormondroyd, W. J. Handley, M. P. Hobson +1

We provide a nested sampling analysis of the combination of CMB lensing experiments with other cosmological measurements. Nested samples can be used to compute global consistency s…

astro-ph.CO2025

Dynamic or Systematic? Bayesian model selection between dark energy and supernova biases

A. N. Ormondroyd, W. J. Handley, M. P. Hobson +2

The Dark Energy Survey 5-year (DES-5Y) supernovae, combined with Dark Energy Spectroscopic Instrument (DESI) baryon acoustic oscillations, appear to favour Chevallier-Polarski-Lind…

astro-ph.CO2025

Comparison of dynamical dark energy with ΛCDM in light of DESI DR2

A. N. Ormondroyd, W. J. Handley, M. P. Hobson +1

We present an updated reconstruction of the dark energy equation of state, , using the newly released DESI DR2 Baryon Acoustic Oscillation (BAO) data in combination with Pant…