Fundamental cosmology from ANDES precision spectroscopy
arXiv:2305.01446 · doi:10.1093/mnras/stad1359
Abstract
Fundamental cosmology observations, such as the detection of the redshift drift and tests of the universality of physical laws, are key science and design drivers of the ArmazoNes high Dispersion Echelle Spectrograph (ANDES), an Extremely Large Telescope instrument. While separate forecasts for each of them have been reported, we have developed Fisher Matrix based forecast tools combining both of these observables. We demonstrate the synergies between the two ANDES datasets, quantifying the improvements in cosmology and fundamental physics parameter constraints for two separate theoretical paradigms. We publicly release this forecast code, which is one of the tools for the optimisation of the ANDES observing strategy.
arXiv comment8 pages, 3 figures, 2 tables, MNRAS (in press)
References in corpus (26)
- Exploring the Expansion History of the Universe
- Accelerating Universes with Scaling Dark Matter
- Cosmic dynamics in the era of Extremely Large Telescopes
- Improved limits for violations of local position invariance from atomic clock comparisons
- Evolution of the Fine Structure Constant Driven by Dark Matter and the Cosmological Constant
- The status of varying constants: a review of the physics, searches and implications
- Exploring the Dark Energy Redshift Desert with the Sandage-Loeb Test
- The time evolution of cosmological redshift as a test of dark energy
- Fundamental physics with ESPRESSO: Precise limit on variations in the fine-structure constant towards the bright quasar HE 05154414
- Toward a Direct Measurement of the Cosmic Acceleration
- Fundamental physics with Espresso: Towards an accurate wavelength calibration for a precision test of the fine-structure constant
- Probing dark energy with redshift-drift
- Constraining Variations in the Fine Structure Constant in the presence of Early Dark Energy
- Forecasts of redshift drift constraints on cosmological parameters
- Euclid: constraining dark energy coupled to electromagnetism using astrophysical and laboratory data
- The spectroscopic follow-up of the QUBRICS bright quasar survey
- The ACCELERATION programme: I. Cosmology with the redshift drift
- Redshift drift cosmography with ELT and SKAO measurements
- Spectroscopy of QUBRICS quasar candidates: 1672 new redshifts and a Golden Sample for the Sandage Test of the Redshift Drift
- Cosmological impact of redshift drift measurements
- The complementarity of the redshift drift
- Current and future constraints on extended Bekenstein-type models for a varying fine-structure constant
- Forecasting cosmic acceleration measurements using the Lyman- forest
- Constraints on extended Bekenstein models from cosmological, astrophysical, and local data
- Fundamental physics with ESPRESSO: Constraints on Bekenstein and dark energy models from astrophysical and local probes
- Distinguishing freezing and thawing dark energy models through measurements of the fine-structure constant