#GW250114's
#GW250114's source is much like that for our first detection GW150914. Progress with our detectors means that the signal is much louder. Therefore, we can make much better measurements

📊: doi.org/10.1103/kw5g...

#O4IsHere
September 10, 2025 at 5:09 PM
GW250114: Precision Test of Einstein’s No?Hair Theorem and Hawking’s Area Law
https://ripley.guru/main/article/gw_precision_test_einstein_hawki
ng
September 12, 2025 at 1:18 AM
The New York Times shares celebrations of our 10 year anniversary, and the challenges ahead, with memories of Rai Weiss and our clearest detection #GW250114

www.nytimes.com/2025/09/10/s... by Dennis Overbye

#GW10Years 🔭 🧪 ⚛️ ☄️
September 15, 2025 at 1:16 PM
Catch up with everything you need to know about our latest #GravitationalWave discovery #GW250114 with our infographics

Credit: Sanika Khadkikar/Penn State & Lucy Reading-Ikkanda/Simons Foundation

#O4IsHere 🔭🧪⚛️☄️
September 11, 2025 at 2:07 AM
What a way to celebrate ten years of gravitational wave astronomy!

This incredible discovery was made by both LIGO detectors. Let’s hope we can keep them both in operation 🤞

www.nytimes.com/2025/09/10/s...

#GW10Years #GW250114
Happy Birthday, LIGO. Now Drop Dead.
www.nytimes.com
September 26, 2025 at 12:56 AM
I appreciate the poetic vibe, but let’s focus on GW250114: black holes aren’t “engines,” rather they’re cosmic heavyweights. GW250114’s merger confirmed Einstein’s predictions.
Our galaxy’s supermassive black hole shapes its structure, but it’s not our “destination.”
September 30, 2025 at 5:50 PM
GW250114 reveals signatures of post-merger black-hole horizon
Oshita, N., Ma, S., Chen, Y. & Yang, H. Probing direct waves in black hole ringdowns. Preprint at https://arxiv.org/abs/2509.09165 (2025). Abac, A. G. et al. GW250114: testing Hawking’s area law and the Kerr nature of black holes. Phys. Rev. Lett. 135, 111403 (2025). Akiyama, K. et al. First M87 Event Horizon Telescope results. I. The shadow of the supermassive black hole. Astrophys. J. Lett. 875, L1 (2019). Reynolds, C. S. Measuring black hole spin using X-ray reflection spectroscopy. Space Sci. Rev. 183, 277–294 (2014). Blandford, R. D. & Znajek, R. L. Electromagnetic extraction of energy from Kerr black holes. Mon. Not. R. Astron. Soc. 179, 433–456 (1977). Aasi, J. et al. Advanced LIGO. Class. Quantum Gravity 32, 074001 (2015). Acernese, F. et al. Advanced Virgo: a second-generation interferometric gravitational wave detector. Class. Quantum Gravity 32, 024001 (2014). Akutsu, T. et al. Overview of KAGRA: detector design and construction history. Prog. Theor. Exp. Phys. 2021, 05A101 (2020). The LIGO Scientific Collaboration, the Virgo Collaboration & the KAGRA Collaboration. GWTC-4.0: updating the gravitational-wave transient catalog with observations from the first part of the fourth LIGO–Virgo–KAGRA observing run. Preprint at https://arxiv.org/abs/2508.18082 (2025). Teukolsky, S. A. Perturbations of a rotating black hole. I. Fundamental...
www.nature.com
June 25, 2026 at 7:25 AM
14 Septembre 2015 - 14 Janvier 2025 : quand la théorie de l'aire du trou noir fusionné se confirme ! (découvert par S. Hawking et “entendu” par #LIGO...)

blog.sosordi.net/2025/09/14-s...

#TrouNoirFusionne #GW250114
September 12, 2025 at 2:19 PM
The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration, A. G. Abac, I. Abouelfettouh, F. Acernese, K. Ackley, C. Adamcewicz, S. Adhicary, D. Adhikari, ...
GW250114: testing Hawking's area law and the Kerr nature of black holes
https://arxiv.org/abs/2509.08054
September 11, 2025 at 6:20 AM
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That’s the magic of LIGO!
No close-up views needed to test the no-hair theorem—gravitational waves are a cosmic fingerprint. GW250114’s vibrations (247 Hz main tone, 249 Hz overtone) match Einstein’s predictions within ±30%, proving black holes are simple, ...
September 30, 2025 at 6:23 PM