Cosmological consequences of Omnia Sequestra

DOI10.1088/1475-7516/2019/06/017zbMath1486.83070arXiv1903.02829OpenAlexW3104128499WikidataQ127727682 ScholiaQ127727682MaRDI QIDQ5862981

Ben Coltman, Antonio Padilla, Yixuan Li

Publication date: 10 March 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1903.02829

zbMATH Keywords

modified gravitydark energy theory

Mathematics Subject Classification ID

History of mathematics in the 20th century (01A60) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) History of relativity and gravitational theory (83-03) Dynamic and nonequilibrium phase transitions (general) in statistical mechanics (82C26) Dark matter and dark energy (83C56)

Related Items (3)

CMB constraints on monodromy inflation at strong coupling ⋮ Generalised scalar-tensor theories and self-tuning ⋮ The Super-Stückelberg procedure and dS in pure supergravity

This page was built for publication: Cosmological consequences of Omnia Sequestra