activity
19972026
most citedDynamical dark energy in light of the latest observations

497 citations · 8.4k across the 112 of their papers we have counts for

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Showing 2020Show all

6 papers · 1 filter

astro-ph.CO2020★ 81 cited

Recombination-independent determination of the sound horizon and the Hubble constant from BAO

Levon Pogosian, Gong-Bo Zhao, Karsten Jedamzik

The Hubble tension and attempts to resolve it by modifying the physics of (or at) recombination motivate finding ways to determine and the sound horizon at the epoch of baryo…

astro-ph.CO2020★ 212 cited

Why reducing the cosmic sound horizon alone can not fully resolve the Hubble tension

Karsten Jedamzik, Levon Pogosian, Gong-Bo Zhao

The mismatch between the locally measured expansion rate of the universe and the one inferred from the cosmic microwave background measurements by Planck in the context of the stan…

astro-ph.CO2020★ 271 cited

CMB-S4: Forecasting Constraints on Primordial Gravitational Waves

S4 Collaboration, Kevork Abazajian, Graeme E. Addison +233

CMB-S4---the next-generation ground-based cosmic microwave background (CMB) experiment---is set to significantly advance the sensitivity of CMB measurements and enhance our underst…

astro-ph.CO2020★ 217 cited

Relieving the Hubble tension with primordial magnetic fields

Karsten Jedamzik, Levon Pogosian

The standard cosmological model determined from the accurate cosmic microwave background measurements made by the Planck satellite implies a value of the Hubble constant that…

astro-ph.IM2020

The Case for Probe-class NASA Astrophysics Missions

Martin Elvis, Jon Arenberg, David Ballantyne +45

Astrophysics spans an enormous range of questions on scales from individual planets to the entire cosmos. To address the richness of 21st century astrophysics requires a correspond…

hep-ph2020★ 41 cited

Decay of Cosmic Global String Loops

Ayush Saurabh, Tanmay Vachaspati, Levon Pogosian

We numerically study the decay of cosmic global string loops due to radiation of Goldstone bosons and massive scalar () particles. The length of loops we study range from 200-10…