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20242026
most citedDESI Dark Energy Time Evolution is Recovered by Cosmologically Coupled Black Holes

25 citations · 26 across the 4 of their papers we have counts for

collaborators

6 papers

gr-qc2026

A Strong Cosmologically Coupled Mass Growth Solution in Linearized General Relativity

Kevin S. Croker, Joshua Cohon, Viktor T. Toth +13

DESI Data Release 2 has heightened interest in cosmologically coupled black holes (CCBHs) as an explanation for accelerating late-time expansion, but known models for CCBHs grow to…

hep-ph2026

Dark Radiation Sticks Together: Dark QCD and the Hubble Tension

Matthew R. Buckley, Nicolas Fernandez, Eric Putney

We introduce a model of dark matter charged under a new confining gauge group akin to the Standard Model's quantum chromodynamics (QCD). The fermionic sector contains both heavy an…

astro-ph.CO2025★ 1 cited

General Constraints on Isocurvature from the CMB and Ly- Forest

Matthew R. Buckley, Peizhi Du, Nicolas Fernandez +1

Current cosmological data are well-described by the Lambda-Cold Dark Matter (CDM) model, which assumes adiabatic initial conditions for the primordial density perturbations. Thi…

hep-ph2024

Force-feeding Supermassive Black Holes with Dissipative Dark Matter

Matthew R. Buckley, Nicolas Fernandez

Supermassive black holes with masses have been discovered by JWST at high redshifts (). It is difficult to explain such objects as the result of ac…

astro-ph.CO2024★ 25 cited

DESI Dark Energy Time Evolution is Recovered by Cosmologically Coupled Black Holes

Kevin S. Croker, Gregory Tarlé, Steve P. Ahlen +4

Recent baryon acoustic oscillation (BAO) measurements by the Dark Energy Spectroscopic Instrument (DESI) provide evidence that dark energy (DE) evolves with time, as parameterized…

hep-ph2024

Dark Radiation Isocurvature from Cosmological Phase Transitions

Matthew R. Buckley, Peizhi Du, Nicolas Fernandez +1

Cosmological first order phase transitions are typically associated with physics beyond the Standard Model, and thus of great theoretical and observational interest. Models of phas…