Cosmological Models Are In Trouble After Recent Studies on Dark Energy - YouTube
https://www.youtube.com/watch?v=NK-4TViTilU

Cosmological Models Are In Trouble After Recent Studies on Dark Energy - YouTube
https://www.youtube.com/watch?v=NK-4TViTilU


We report the first measurement of the Hubble constant $H_0$ using the stochastic gravitational-wave background arising from binary black hole mergers. This astrophysical background is sensitive to the expansion history of the Universe and thus can be used for cosmological parameter inference independently of not only electromagnetic methods, but also gravitational-wave standard siren approaches. We describe the background's cosmological dependence and show how it can be used as a ``stochastic siren'' to measure $H_0$. By analyzing existing resolved binary black hole mergers and the current non-detection of the background, we find that $H_0$ can be measured more accurately relative to using resolved mergers alone. We also note that the stochastic siren may serve a unique role in the Hubble tension in that the lower bound of the $H_0$ measurement would progressively increase with continued non-detection of the background.
New Method Uses Gravitational Waves to Improve Measurements of the Universe's Expansion
📰 Original title: A faint cosmic hum could solve the Universe’s expansion mystery
🤖 IA: It's not clickbait ✅
👥 Usuarios: It's not clickbait ✅
View full AI summary: https://killbait.com/en/new-method-uses-gravitational-waves-to-improve-measurements-of-the-universes-expansion/?redirpost=4e6ee84f-05b8-4f2c-ba0b-ad2d64423b1d
#science #gravitationalwaves #universeexpansion #hubbleconstant

Astronomers have long known that the universe is expanding, but the exact rate of expansion, measured by the Hubble constant, remains a mystery. Multiple methods used to calculate this constant have…
Munich astronomers imaged and modelled an exceptionally rare #supernova that could provide a new, independent way to measure how fast the #universe is expanding: http://go.tum.de/991366 🌌
#hubbleconstant #cosmicexpansion #cosmology #astrophysics
📷C. Saulder
Join us for the latest lecture of "Wissenschaft für Alle"!
What is the #HubbleConstant and how is it determined? Find out with Andreas Flörs (GSI/FAIR) 🌌
German only.
Online or on site as usual: Wednesday, 25 February 2026, 2 PM
Online event: https://gsi-fair.zoom.us/j/98465545116#success
Meeting-Code: wfa
On site registration: https://indico.gsi.de/event/23430/registrations/7199/
Location: GSI/FAIR #Darmstadt
© NASA, ESA, CSA, STScI
#lecture #science #WissenschaftfürAlle #WfA #particleaccelerator #space
Prof. Wendy Freedman recognized with 2026 Franklin Institute Award in Physics
Pioneering cosmologist honored for landmark measurements of the Hubble Constant.
https://news.uchicago.edu/story/prof-wendy-freedman-recognized-2026-franklin-institute-award-physics
#Cosmology #WendyFreedman #HubbleConstant #Astronomy #Astrophysics #Astrodon #science #news #UChicago
My beautiful star charts that I made to map the Universe. Hint: we're in the middle.
Feast your eyes.
#hubbleconstant
#naturaldisasterchannel
#globalwomensheritagefund
#tibees
#MastoArt
#AIDebate
#runnymede
In this paper, the suitability of fast-declining Type Ia supernovae (SNe Ia) as cosmological standard candles is examined utilizing a Hubble Flow sample of 43 of these objects observed by the Carnegie Supernova Project (CSP). We confirm previous suggestions that fast-declining SNe Ia offer a viable method for estimating distances to early-type galaxies when the color-stretch parameter, $s_{BV}$, is used as a measure of the light curve shape. As a test, we employ the Tripp (1998) method, which models the absolute magnitude at maximum as a function of light curve shape and color. We calibrate the sample using 12 distance moduli based on published Infrared Surface Brightness Fluctuations to derive a value of the Hubble constant that is in close agreement with the value found by Uddin et al. (2024), using the same methodology, but with the full sample of CSP SNe Ia. We also develop a new and simple method of estimating the distances of fast decliners only based on their colors at maximum (and not light curve shape) and find that it has a precision similar to the Tripp method. This "Color" technique is a powerful tool that is unique to fast-declining SNe Ia. We show that the colors of the fast decliners at maximum light are strongly affected by photospheric temperature differences and not solely due to dust extinction, and provide a physical rationale for this effect.
The Perfect Host: JWST Cepheid Observations in a Background-Free SN Ia Host Confirm No Bias in Hubble-Constant Measurements
by Adam Riess and co-authors
https://arxiv.org/abs/2509.01667