A year ago, v. 2 of the paper "Inflation: Theory & Observations" was released, further intensifying my fascination for Inflationary Cosmology. My gratitude goes to @GuiLeiPimentel , Wallisch & Wu; I had the honor of being listed in the Endorsers section.
https://t.co/k5UwYVXZVe
Daniel Baumann (@DD_Baumann) lecture notes on Cosmological Correlations from the BUSSTEP Sept 2026 summer school. Includes 2 problem sets and several reference materials. Notes written together with Austin Joyce.
https://t.co/CP1TDPQUXh
school webpage: https://t.co/MJtUDzFL60
"I don't see why they can't just combine Pantheon+ and DES-Dovekie and get even tighter dark energy constraints"
Your wish is granted!
Featuring @tamarastro@astrojason20 & Ryan Camilleri
https://t.co/WSNUDj4N1d
The “perfect cosmological principle” isn’t true for our Universe
On the largest scales, the Universe is the same everywhere in space.
Could it also be the same everywhere in time?
That's the Perfect Cosmological Principle: fascinating, but untrue.
https://t.co/9m9xYmooBV
1/ 📄 New paper’s out: we study phase coherence in primordial #cosmology.
The sharp acoustic peaks of the CMB and their late-time imprint in BAO require primordial perturbations to oscillate with extremely coherent phases.
What fixes this coherence? 🧵
https://t.co/fEbeMnbLyT
Is the Universe truly infinite in size?
The observable Universe is "only" 13.8 billion years old, extending for 46 billion light-years in all directions.
But what about the unobservable Universe?
It could still be infinite!
https://t.co/ZJooej5O7H
Fascinated by recent evidence for evolving dark energy?
But wondering what it all means for fundamental physics models?
Cosmology Talks has you covered!
Everything you need to know about single scalar field dark energy in 2026
https://t.co/egx8mxRXJJ
Growth, geometry, and early-universe split of the matter density parameter Ωₘ
Felicitas Keil, Isaac Tutusaus, Alain Blanchard
https://t.co/pn6e4oxrpF [𝚊𝚜𝚝𝚛𝚘-𝚙𝚑.𝙲𝙾]
Signals from the early Universe: a comprehensive search for primordial features in Planck CMB datasets
Antonio Raffaelli, Mario Ballardini, Nicola Barbieri
https://t.co/rqs9oLwmoJ [𝚊𝚜𝚝𝚛𝚘-𝚙𝚑.𝙲𝙾]
Cosmology from HI galaxy surveys with the SKA
Ainulnabilah Nasirudin, Philip Bull, Ziad Sakr, Joël Mayor, Benedict Bahr-Kalus, Hengxing Pan, Stefano Camera, José Fonseca, Liantsoa F. Randrianjanahary, Gabriella De Lucia, …
https://t.co/MW76vSVGiY [𝚊𝚜𝚝𝚛𝚘-𝚙𝚑.𝙲𝙾]
Latest DESI (+CMB +SN) data got you spooked? Seeing ghosts and *phantoms*?
Don't panic!
@Primeval_Arhsim is here to reassure you: "No phantoms are needed by current observational cosmology"
https://t.co/e8Trb1vlFD
Hope you enjoy watching this latest release on Cosmology Talks, where Shaun & I discuss about Interpretation of Evolving Dark Energy from Cosmological observations, including Phantom & Phantom-crossing behavior: in the context of DESI results & beyond. (Based on my new paper) ✨
1/3] What is Dynamical Phantom Dark Energy? Absolutely delighted to have received many +ve feedbacks from Cosmology colleagues: both theorists & observers! Sharing here again for wider reach. Hope U find it informative; Happy to discuss more. YouTube link: https://t.co/hR0UIC6Jj2
In a study published today in Nature, two researchers argue galaxies align in enormous filaments even on scales where the cosmos should appear smooth and uniform.
https://t.co/rxKAijejOc
#Cosmology@Nature@ScienceMagazine@fsyloslab
Sobre la ecuación de estado del sector oscuro: https://t.co/KDKgKFzCon La posible variación de la densidad de energía oscura a lo largo de la historia cósmica, y la pregunta acerca de la posible variación de la ecuación de estado de la materia oscura.