Results 101 to 110 of about 279,601 (204)

Electrobaryonic axion: hair of neutron stars

Journal of High Energy Physics
Axion-like particles are predicted in many physics scenarios beyond the Standard Model (SM). Their interactions with SM particles may arise from the triangle anomaly of the associated global symmetry, along with other SM global and gauge symmetries ...
Yang Bai, Carlos Henrique de Lima
doaj   +1 more source

Discovery of a radio emitting neutron star with an ultra-long spin period of 76 seconds. [PDF]

Nat Astron, 2022
Caleb M, Heywood I, Rajwade K, Malenta M, Stappers B, Barr E, Chen W, Morello V, Sanidas S, van den Eijnden J, Kramer M, Buckley D, Brink J, Motta SE, Woudt P, Weltevrede P, Jankowski F, Surnis M, Buchner S, Bezuidenhout MC, Driessen LN, Fender R.   +21 more
europepmc   +1 more source

Detection of Simultaneous Quasiperiodic Oscillation Triplets in 4U 1728-34 and Constraining the Neutron Star Mass and Moment of Inertia

The Astrophysical Journal
We report simultaneous detection of twin kHz and ∼40 Hz quasiperiodic oscillations (QPOs) in the time-resolved analysis of the AstroSat/LAXPC observation of the neutron star low-mass X-ray binary, 4U 1728-34.
Kewal Anand, Ranjeev Misra, J. S. Yadav, Pankaj Jain, Umang Kumar, Dipankar Bhattacharya   +5 more
doaj   +1 more source

X-Rays Radiation of a Neutron Star as a Result of Gas Accretion [PDF]

, 1968
Ja. B. Zel’dovič
openalex   +1 more source

On the Dynamical Evolution of the Asteroid Belt in a Massive Star–Neutron Star Binary

The Astrophysical Journal
Some fast radio bursts (FRBs) exhibit repetitive behaviors, and their origins remain enigmatic. It has been argued that repeating FRBs could be produced by the interaction between a neutron star and an asteroid belt.
Chen Deng, Yong-Feng Huang, Chen Du, Pei Wang, Zi-Gao Dai   +4 more
doaj   +1 more source

Accretion in supergiant High Mass X-ray Binaries

EPJ Web of Conferences, 2014
Supergiant High Mass X-ray Binary systems (sgHMXBs) consist of a massive, late type, star and a neutron star. The massive stars exhibits strong, radiatively driven, stellar winds.
Manousakis Antonios, Walter Roland, Blondin John   +2 more
doaj   +1 more source

Accretion onto a small black hole at the center of a neutron star. [PDF]

Phys Rev D, 2021
Richards CB, Baumgarte TW, Shapiro SL.
europepmc   +1 more source

Neutron Star Structure from Pulsar Observations [PDF]

, 1974
David Pines, J. Shaham, M. Ruderman
openalex   +1 more source

Nuclear astrophysics in our time: supernovae, neutron stars and binary neutron star mergers. [PDF]

Eur Phys J Spec Top, 2021
Bandyopadhyay D.
europepmc   +1 more source

Instability of Neutron Star Matter for Pion Condensation [PDF]

, 1975
Akira Suzuki, Y. Futami, Y. Takahashi
openalex   +1 more source