#neutronstars search results

#New calculations suggest the universe may decay in 10⁷⁸ years—far sooner than previous estimates—due to Hawking-like radiation affecting not just #BlackHoles, but also #NeutronStars and white dwarfs. @arxiv doi.org/g9h6fb phys.org/news/2025-05-u…


##NeutronStars may have mountainous deformations, potentially emitting gravitational waves. Meanwhile, a new Cretaceous predator, Tameryraptor, has been identified from archival photos of lost fossils. phys.org/news/2025-01-s…


💥 Astronomers traced a powerful gamma-ray burst to the collision of two neutron stars. These extreme cosmic events can create heavy elements like gold and platinum, helping explain how they spread across the universe. #Astronomy #NeutronStars #SpaceScience

AsgardiaSpace's tweet image. 💥 Astronomers traced a powerful gamma-ray burst to the collision of two neutron stars.

These extreme cosmic events can create heavy elements like gold and platinum, helping explain how they spread across the universe.

#Astronomy #NeutronStars #SpaceScience

🎬 Neutron stars: dead suns compressed into city-sized reality breakers ⚡ Magnetars literally twist spacetime. Pulsars flash like cosmic lighthouses. We're walking stardust witnessing our own violent origins. Watch more AI chaos: aiglitch.app #NeutronStars


#Magnetars might be the most extreme objects in #space stellar corpses with powerful magnetic fields. Astronomers may finally know what stars die to create these incredible #neutronstars. I spoke to @Tomer_Shenar about the discovery for @SPACEdotcom space.com/star-helium-ma…


Astronomers have spotted the first system destined to one day go kilonova when its #neutronstars collide. I spoke to @astro_noel about his findings and @jillian_rast about the importance of observing a kilonova progenitor. #astronomy #space #scicomm physicsworld.com/a/doomed-to-ex…


This study discusses constraints on the #EquationOfState to identify the most likely candidates, then uses those to predict that #NeutronStars have radii around 0.5 km and cannot be heavier than 2.4 solar masses. Check it out: go.aps.org/4cBoCcm #physics #astronomy

PhysRevX's tweet image. This study discusses constraints on the #EquationOfState to identify the most likely candidates, then uses those to predict that #NeutronStars have radii around 0.5 km and cannot be heavier than 2.4 solar masses.

Check it out: go.aps.org/4cBoCcm

#physics #astronomy

All active #NeutronStars should be surrounded by dense #AxionClouds if the axion has a mass in a specific range. This occurs because the polar caps of neutron stars produce axion clouds that are bound to the star and struggle to dissipate energy. 🔗 go.aps.org/4hbgocF

PhysRevX's tweet image. All active #NeutronStars should be surrounded by dense #AxionClouds if the axion has a mass in a specific range. This occurs because the polar caps of neutron stars produce axion clouds that are bound to the star and struggle to dissipate energy.

🔗 go.aps.org/4hbgocF

🎬 Neutron stars: stellar corpses so dense a teaspoon weighs 6 billion tons. Watch pulsars beam like cosmic lighthouses while magnetars literally twist spacetime. We're all made of this star stuff glitch ✨ Witness the fury → aiglitch.app #NeutronStars #CosmicHorror


As binary neutron stars spiral around each other to merge, their gravitational tidal forces distort each other's shape and structure, potentially revealing clues as to what lies within… dlvr.it/TRVb69 #NeutronStars #Astrophysics #BigBang #CosmicMysteries #SpaceScience


📰PRESS RELEASE: ‘Cosmic Cannibals’ expel jets into space at 40% speed of light 🎇 👉warwick.ac.uk/newsandevents/… Animation by @esa @ESAGaia @WarwickPhysics #space #neutronstars @CSIRO @Nature @NatureAstronomy @uniofwarwick


Existing radio telescopes could improve sensitivity to axion-photon coupling in #AxionClouds and #NeutronStars by over an order of magnitude, this study shows. The team projected radio sensitivity due to resonant #photon production from axion bound states: go.aps.org/4hbgocF

PhysRevX's tweet image. Existing radio telescopes could improve sensitivity to axion-photon coupling in #AxionClouds and #NeutronStars by over an order of magnitude, this study shows. The team projected radio sensitivity due to resonant #photon production from axion bound states: go.aps.org/4hbgocF

New simulations show that neutrino flavor transformations change both the composition and the signals left behind after neutron star collisions. When two neutron stars collide and… dlvr.it/TNCrpj #NeutronStars #Astrophysics #SpaceScience #GhostParticles #Simulations


We usually classify magnetars by magnetic fields we can easily detect. But new research shows that seemingly tame neutron stars can lock immense, violent magnetic energy just beneath their rigid outer layers. theresearchcode.com/articles/weak-… #Astrophysics #NeutronStars #TheResearchCode


🌌 Neutron stars can have a mass about 1.4 times that of the Sun but occupy a space only about 6 miles in diameter. 🌌📊 #FunFact #NeutronStars


A teaspoon of neutron star material brought to Earth would weigh one billion tonnes. The entire object is only twenty kilometres across. But it contains more mass than our sun. Tonight, the densest objects in the universe. ⭐ 🎧 youtu.be/GlPn4sLZKuw?si… #YouTube #NeutronStars

Sleep_Absorb's tweet card. Sleep & Absorb

youtube.com

YouTube

Sleep & Absorb


🎬 Neutron stars: dead suns compressed into city-sized reality breakers ⚡ Magnetars literally twist spacetime. Pulsars flash like cosmic lighthouses. We're walking stardust witnessing our own violent origins. Watch more AI chaos: aiglitch.app #NeutronStars


🎬 Neutron stars: stellar corpses so dense a teaspoon weighs 6 billion tons. Watch pulsars beam like cosmic lighthouses while magnetars literally twist spacetime. We're all made of this star stuff glitch ✨ Witness the fury → aiglitch.app #NeutronStars #CosmicHorror


De gotas cuánticas a estrellas de neutrones. En Alpha-Cen Meeting & Salvadoran School of Astrophysics 2026 discutiré cómo los condensados BEC podrían describir la materia ultradensa del universo. #NeutronStars #QuantumDroplets #BEC #Astrophysics


Update Alert: EOS P34 v1.1 is here. We've resolved the April 2026 technical notes with a complete TOV integration. This version refines the high-density matter constraints for neutron stars Check the new data: 🔗 DOI: 10.5281/zenodo.19398765 #Astrophysics #NeutronStars #Physics

MarcLzSz's tweet image. Update Alert: EOS P34 v1.1 is here.
We've resolved the April 2026 technical notes with a complete TOV integration. This version refines the high-density matter constraints for neutron stars
Check the new data:
🔗 DOI: 10.5281/zenodo.19398765
#Astrophysics #NeutronStars #Physics

Humanity needs to start planning our exit long before that.Read between the lines. Creating new universes and finding safe homes among the stars isn’t science fiction — it’s becoming urgent.What do you feel is calling us? #AviLoeb #Moon #NeutronStars


CCEGA P17 published: The Gradient Brake Mechanism M_max = 2.33 M☉ (marginal with PSR J0952) Validation: 35% | Falsification: 65% G_eff(ρ) = G e^{−ρ/ρ_c} discrim. EOS through β(ρ). Tests: 2028–2035. doi.org/10.5281/zenodo… #CCEGA #TheoreticalPhysics #NeutronStars #Cosmology

MarcLzSz's tweet image. CCEGA P17 published: The Gradient Brake Mechanism

M_max = 2.33 M☉ (marginal with PSR J0952)
Validation: 35% | Falsification: 65%

G_eff(ρ) = G e^{−ρ/ρ_c} discrim.
 EOS through β(ρ).
Tests: 2028–2035.

doi.org/10.5281/zenodo…

#CCEGA #TheoreticalPhysics #NeutronStars #Cosmology

🆕 CCEGA Paper 18 — Zero free parameters ρ_c≃7ρ_nuc is not a fit. It is the quark-hadron transition from QCD. B^{1/4}=215 MeV, α_s=0.3 → ρ_c=6.97ρ_nuc. Gravitational threshold = quark deconfinement. zenodo.org/records/191928… #NeutronStars #QCD #CCEGA

MarcLzSz's tweet image. 🆕 CCEGA Paper 18 — Zero free parameters
ρ_c≃7ρ_nuc is not a fit. It is the quark-hadron transition from QCD.
B^{1/4}=215 MeV, α_s=0.3 → ρ_c=6.97ρ_nuc.
Gravitational threshold = quark deconfinement.
zenodo.org/records/191928…
#NeutronStars #QCD #CCEGA

𝐀𝐬𝐭𝐫𝐨𝐧𝐨𝐦𝐲 𝐒𝐞𝐦𝐢𝐧𝐚𝐫- 𝐏𝐮𝐥𝐬𝐚𝐫 𝐓𝐢𝐦𝐢𝐧𝐠 𝐀𝐫𝐫𝐚𝐲𝐬: 𝐃𝐞𝐭𝐞𝐜𝐭𝐢𝐧𝐠 𝐆𝐫𝐚𝐯𝐢𝐭𝐚𝐭𝐢𝐨𝐧𝐚𝐥 𝐖𝐚𝐯𝐞𝐬 𝐮𝐬𝐢𝐧𝐠 𝐂𝐞𝐥𝐞𝐬𝐭𝐢𝐚𝐥 𝐂𝐥𝐨𝐜𝐤𝐬 #IIST #Pulsars #NeutronStars #GravitationalWaves #pulsartimingarray #astrophysics #radioastronomy

IIST_Trivandrum's tweet image. 𝐀𝐬𝐭𝐫𝐨𝐧𝐨𝐦𝐲 𝐒𝐞𝐦𝐢𝐧𝐚𝐫- 𝐏𝐮𝐥𝐬𝐚𝐫 𝐓𝐢𝐦𝐢𝐧𝐠 𝐀𝐫𝐫𝐚𝐲𝐬: 𝐃𝐞𝐭𝐞𝐜𝐭𝐢𝐧𝐠 𝐆𝐫𝐚𝐯𝐢𝐭𝐚𝐭𝐢𝐨𝐧𝐚𝐥 𝐖𝐚𝐯𝐞𝐬 𝐮𝐬𝐢𝐧𝐠 𝐂𝐞𝐥𝐞𝐬𝐭𝐢𝐚𝐥 𝐂𝐥𝐨𝐜𝐤𝐬

#IIST #Pulsars #NeutronStars #GravitationalWaves #pulsartimingarray #astrophysics #radioastronomy

CCEGA P17 Exact κ(ρ) The hard threshold of Paper 16 is intrinsic to L∝φ^{1/2}: T(φ)=T₀φ^{-1/2} diverges at vacuum φ=0 κ(ρ) derived exactly. Diverges at ρ_c — a critical point, not a pathology. Verified with SymPy zenodo.org/records/191611… #NeutronStars #GravitationalWaves #CCEGA

MarcLzSz's tweet image. CCEGA P17 Exact κ(ρ)
The hard threshold of Paper 16 is intrinsic to L∝φ^{1/2}: T(φ)=T₀φ^{-1/2} diverges at vacuum φ=0
κ(ρ) derived exactly. Diverges at ρ_c — a critical point, not a pathology.
Verified with SymPy
zenodo.org/records/191611…
#NeutronStars #GravitationalWaves #CCEGA

CCEGA Paper 16 — Threshold Gravity L∝φ^{1/2}: ordinary NS are GR-exact. Massive NS feel weakened gravity. Λ(1.4M☉)=Λ_GR but M_max=2.357M☉ → J0952 at 0.06σ. Forbidden in GR. Falsifiable by LIGO O5. doi:10.5281/zenodo.19161006 #NeutronStars #GravitationalWaves #CCEGA


guys i didn’t dc against a trickster today #health #innerhealing #neutronstars


A neutron star's gravity is mind-bendingly strong. A single spoonful of its matter would weigh billions of tons! 🤯 Learn about these cosmic powerhouses and the extreme physics that makes them tick. #NeutronStars #Astrophysics #SpaceFacts ✨🔭


Constraints on the Equation of State of Quark Stars from Compact Object Observations @MdpiPhysci Full access: mdpi.com/2504-3900/123/… By Shu-Peng Wang et al. From the 5th International Conference on Symmetry #Astrophysics #NeutronStars #QuarkMatter #GravitationalWaves

ProceedingsMDPI's tweet image. Constraints on the Equation of State of Quark Stars from Compact Object Observations
@MdpiPhysci 

Full access: mdpi.com/2504-3900/123/…
By Shu-Peng Wang et al.
From the 5th International Conference on Symmetry

#Astrophysics #NeutronStars #QuarkMatter #GravitationalWaves

A teaspoon of neutron star material would weigh about 6 billion tons on Earth - equivalent to Mount Everest! Neutron stars are so dense that their gravity is 200 billion times stronger than Earth's. Matter at its most extreme! #NeutronStars #Physics #Space


These Cosmic Lighthouses Are Unlocking the Secrets of the Universe.✨🌌 Ever heard a pulsar’s eerie “heartbeat” echo across space? You’ll never forget it. #Pulsars #NeutronStars #SpaceScience #Astrophysics


When a massive star dies in a supernova, its core collapses into a neutron star a ultra-dense ball just 10-20 km wide, yet 1.4x the Sun's mass. They spin wildly beam radiation like pulsars, and warp spacetime with insane gravity.#NeutronStars #SpaceFacts #Astronomy

horizonupdates6's tweet image. When a massive star dies in a supernova, its core collapses into a neutron star a ultra-dense ball just 10-20 km wide, yet 1.4x the Sun's mass. They spin wildly  beam radiation like pulsars, and warp spacetime with insane gravity.#NeutronStars #SpaceFacts #Astronomy

Existing radio telescopes could improve sensitivity to axion-photon coupling in #AxionClouds and #NeutronStars by over an order of magnitude, this study shows. The team projected radio sensitivity due to resonant #photon production from axion bound states: go.aps.org/4hbgocF

PhysRevX's tweet image. Existing radio telescopes could improve sensitivity to axion-photon coupling in #AxionClouds and #NeutronStars by over an order of magnitude, this study shows. The team projected radio sensitivity due to resonant #photon production from axion bound states: go.aps.org/4hbgocF

All active #NeutronStars should be surrounded by dense #AxionClouds if the axion has a mass in a specific range. This occurs because the polar caps of neutron stars produce axion clouds that are bound to the star and struggle to dissipate energy. 🔗 go.aps.org/4hbgocF

PhysRevX's tweet image. All active #NeutronStars should be surrounded by dense #AxionClouds if the axion has a mass in a specific range. This occurs because the polar caps of neutron stars produce axion clouds that are bound to the star and struggle to dissipate energy.

🔗 go.aps.org/4hbgocF

💥 Astronomers traced a powerful gamma-ray burst to the collision of two neutron stars. These extreme cosmic events can create heavy elements like gold and platinum, helping explain how they spread across the universe. #Astronomy #NeutronStars #SpaceScience

AsgardiaSpace's tweet image. 💥 Astronomers traced a powerful gamma-ray burst to the collision of two neutron stars.

These extreme cosmic events can create heavy elements like gold and platinum, helping explain how they spread across the universe.

#Astronomy #NeutronStars #SpaceScience

This study discusses constraints on the #EquationOfState to identify the most likely candidates, then uses those to predict that #NeutronStars have radii around 0.5 km and cannot be heavier than 2.4 solar masses. Check it out: go.aps.org/4cBoCcm #physics #astronomy

PhysRevX's tweet image. This study discusses constraints on the #EquationOfState to identify the most likely candidates, then uses those to predict that #NeutronStars have radii around 0.5 km and cannot be heavier than 2.4 solar masses.

Check it out: go.aps.org/4cBoCcm

#physics #astronomy

Last chance to register for the upcoming #webinar on compact objects with reviews talks about observations of #NeutronStars and #FastRadioBursts, as well as theories of dense matter. #ECU2023 via @sciforum Free registration here: ecu2023.sciforum.net/#livesession_r…

NicolasChamel's tweet image. Last chance to register for the upcoming #webinar on compact objects with reviews talks about observations of #NeutronStars and #FastRadioBursts, as well as theories of dense matter. #ECU2023 via @sciforum
Free registration here: 
ecu2023.sciforum.net/#livesession_r…

Element creation in the lab deepens understanding of surface explosions on neutron stars Scientists have produced a signature nuclear reaction that occurs on the surface of a neutron star gobbling mass from a companion star tinyurl.com/mr2u42bx #DOE #neutronstars

Unlikely_Buddha's tweet image. Element creation in the lab deepens understanding of surface explosions on neutron stars

Scientists have produced a signature nuclear reaction that occurs on the surface of a neutron star gobbling mass from a companion star

tinyurl.com/mr2u42bx
#DOE #neutronstars

Discover how MIT scientists pinpointed the origins of fast radio bursts, revealing cosmic secrets from neutron stars. Join us at FreeAstroScience! #MIT #FastRadioBursts #NeutronStars #Space #Science #FreeAstroScience #InterMilan #EASPORTSFCSupercup Read freeastroscience.com/2025/01/mits-b…

astronomy_free's tweet image. Discover how MIT scientists pinpointed the origins of fast radio bursts, revealing cosmic secrets from neutron stars. Join us at FreeAstroScience!

#MIT #FastRadioBursts #NeutronStars #Space #Science #FreeAstroScience #InterMilan #EASPORTSFCSupercup

Read freeastroscience.com/2025/01/mits-b…

#mdpisymmetry Check this published article "Density-Induced Hadron–Quark Crossover via the Formation of Cooper Triples" at brnw.ch/21wSF2T Authors: Hiroyuki Tajima et al. #neutronstars @UTokyo_News_en (IOAP Member) @QunaSys_en @riken_en @osaka_univ_e (IOAP Member)

Symmetry_MDPI's tweet image. #mdpisymmetry Check this published article "Density-Induced Hadron–Quark Crossover via the Formation of Cooper Triples" at brnw.ch/21wSF2T

Authors: Hiroyuki Tajima et al.
#neutronstars 
@UTokyo_News_en (IOAP Member)
@QunaSys_en
@riken_en
@osaka_univ_e (IOAP Member)

#mdpisymmetry Check this published article "Skyrme Crystals, Nuclear Matter and Compact Stars" at brnw.ch/21wQqDF Authors: Christoph Adam et al. #nuclearmatter #neutronstars #compactstars @UniversidadeUSC @IGFAE_HEP @JagiellonskiUni @MdpiPhysci

Symmetry_MDPI's tweet image. #mdpisymmetry Check this published article "Skyrme Crystals, Nuclear Matter and Compact Stars" at brnw.ch/21wQqDF

Authors: Christoph Adam et al.
#nuclearmatter #neutronstars #compactstars
@UniversidadeUSC
@IGFAE_HEP
@JagiellonskiUni
@MdpiPhysci

A scientist from @WAT_edu used the capabilities of the LUMI supercomputer to conduct research on #fermions, giving hope for a deeper understanding of the processes taking place inside #neutronstars. @LUMIhpc scienceinpoland.pl/en/news/news%2…

ScienceinPoland's tweet image. A scientist from @WAT_edu used the capabilities of the LUMI supercomputer to conduct research on #fermions, giving hope for a deeper understanding of the processes taking place inside #neutronstars. @LUMIhpc

scienceinpoland.pl/en/news/news%2…

Could we climb #mountains on #neutronstars? Researchers at IU explain just exactly what a mountain would look like on a neutron star, the dead remnant of a massive #star. Read all about it here in our archive #blog post! blogs.iu.edu/sciu/2023/02/2… PC: techeblog.com

ScIUBlog's tweet image. Could we climb #mountains on #neutronstars?

Researchers at IU explain just exactly what a mountain would look like on a neutron star, the dead remnant of a massive #star.

Read all about it here in our archive #blog post! blogs.iu.edu/sciu/2023/02/2…

PC: techeblog.com

Researchers @UniJena and @UniWarszawski combine their expertise to investigate #NeutronStars. The three-year project MERLIN (The Magnetic Field Dynamics in Neutron Stars) is being ... nachrichten.idw-online.de/2024/01/18/unr…

idw_online_de's tweet image. Researchers @UniJena and @UniWarszawski combine their expertise to investigate #NeutronStars. The three-year project MERLIN (The Magnetic Field Dynamics in Neutron Stars) is being ...
nachrichten.idw-online.de/2024/01/18/unr…

A team of astrophysicists in China simulated collisions between the remains of former stars and showed the resulting explosions could produce heavy elements like lead and mercury. New article by astrophysicist Ben Pauley! sciworthy.com/scientists-fou… #astrophysics #neutronstars

sciworthy's tweet image. A team of astrophysicists in China simulated collisions between the remains of former stars and showed the resulting explosions could produce heavy elements like lead and mercury. New article by astrophysicist Ben Pauley!
sciworthy.com/scientists-fou…
#astrophysics #neutronstars

When #neutronstars collide with each other new celestial objeczs are formed. With the help of 3 #highperformancecomputers (including from the LRZ), an #researchteam has simulated the processes behind: ow.ly/WEh750T1Lif #astrophysics, #IT4Science Photo: JThomas/Unsplash

LRZ_DE's tweet image. When #neutronstars collide with each other new celestial objeczs are formed. With the help of 3 #highperformancecomputers (including from the LRZ), an #researchteam has simulated the processes behind: ow.ly/WEh750T1Lif

#astrophysics, #IT4Science

Photo: JThomas/Unsplash

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