Detecting superfluid transition in the pulsar core
Fuente:
arXiv
Guardado en:
| Autores principales: | Bagchi, Partha, Layek, Biswanath, Saini, Dheeraj, Sarkar, Anjishnu, Srivastava, Ajit M., Venkata, Deepthi Godaba |
|---|---|
| Formato: | Preprint |
| Publicado: |
2024
|
| Materias: | |
| Acceso en línea: | |
| Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
Ejemplares similares
Pulsar as a Weber detector of gravitational waves and a probe to its internal phase transitions
por: Bagchi, Partha, et al.
Publicado: (2023)
por: Bagchi, Partha, et al.
Publicado: (2023)
Pulse Modulation as a Signature of the Asteroid-Neutron Star Collision Model for High-Energy Transients
por: Bagchi, Partha, et al.
Publicado: (2026)
por: Bagchi, Partha, et al.
Publicado: (2026)
Large-scale unpinning and pulsar glitches due to the forced oscillation of vortices
por: Layek, Biswanath, et al.
Publicado: (2024)
por: Layek, Biswanath, et al.
Publicado: (2024)
Fastest spinning millisecond pulsars: indicators for quark matter in neutron stars?
por: Gärtlein, Christoph, et al.
Publicado: (2024)
por: Gärtlein, Christoph, et al.
Publicado: (2024)
Orbital eccentricity can make neutron star g-mode resonances observable with current gravitational-wave detectors
por: Takátsy, János, et al.
Publicado: (2026)
por: Takátsy, János, et al.
Publicado: (2026)
First-order phase transitions in the cores of neutron stars
por: Komoltsev, Oleg
Publicado: (2024)
por: Komoltsev, Oleg
Publicado: (2024)
Estimating the dark matter halo velocity and surface temperature of some known pulsars due to dark matter capture
por: Sen, Debashree, et al.
Publicado: (2024)
por: Sen, Debashree, et al.
Publicado: (2024)
MURCA driven Bulk viscosity in neutrino trapped baryonic matter
por: Sarkar, Sreemoyee, et al.
Publicado: (2024)
por: Sarkar, Sreemoyee, et al.
Publicado: (2024)
Correlation between the symmetry energy slope and the deconfinement phase transition
por: Lopes, Luiz L., et al.
Publicado: (2023)
por: Lopes, Luiz L., et al.
Publicado: (2023)
Constraining the competition between the deconfinement and chiral phase transitions in light of the multimessenger era
por: Yuan, Wen-Li, et al.
Publicado: (2024)
por: Yuan, Wen-Li, et al.
Publicado: (2024)
Confronting new NICER mass-radius measurements with phase transition in dense matter and twin compact stars
por: Li, Jia Jie, et al.
Publicado: (2024)
por: Li, Jia Jie, et al.
Publicado: (2024)
Gravitational wave spectrum from first-order QCD phase transitions based on a parity doublet model
por: Gao, Bikai, et al.
Publicado: (2026)
por: Gao, Bikai, et al.
Publicado: (2026)
Detecting the third family of compact stars with normalizing flows
por: Carvalho, Valéria, et al.
Publicado: (2024)
por: Carvalho, Valéria, et al.
Publicado: (2024)
Detecting Hyperons in neutron stars -- a machine learning approach
por: Carvalho, Valéria, et al.
Publicado: (2024)
por: Carvalho, Valéria, et al.
Publicado: (2024)
Perturbative QCD reveals the softening of matter in the cores of massive neutron stars
por: Komoltsev, Oleg
Publicado: (2025)
por: Komoltsev, Oleg
Publicado: (2025)
Axion effects on quark matter and quark-matter cores in massive hybrid stars
por: Liu, He, et al.
Publicado: (2024)
por: Liu, He, et al.
Publicado: (2024)
The diffuse supernova neutrino background: an update with modern population synthesis and core-collapse simulations
por: Lunardini, Cecilia, et al.
Publicado: (2025)
por: Lunardini, Cecilia, et al.
Publicado: (2025)
First detection of X-ray pulsations and spectrum of the high Galactic latitude pulsar PSR J0837-2454 and direct Urca cooling implications
por: Ho, Wynn C. G., et al.
Publicado: (2024)
por: Ho, Wynn C. G., et al.
Publicado: (2024)
Charged-current neutrino opacity within the relativistic Hartree-Fock framework for astrophysical simulations of core-collapse supernovae and binary neutron star mergers
por: Sokołowski, Kamil, et al.
Publicado: (2026)
por: Sokołowski, Kamil, et al.
Publicado: (2026)
The role of ν_τ ultrahigh energy astrophysics in Km^3 detectors
por: Fargion, D.
Publicado: (1997)
por: Fargion, D.
Publicado: (1997)
High density symmetry energy: A key to the solution of the hyperon puzzle
por: Ye, Jun-Ting, et al.
Publicado: (2024)
por: Ye, Jun-Ting, et al.
Publicado: (2024)
Extended Skyrme effective interactions for transport model and neutron stars
por: Wang, Si-Pei, et al.
Publicado: (2023)
por: Wang, Si-Pei, et al.
Publicado: (2023)
Use of the Meta-analysis and Kolmogorov Criteria in the Finding of Singularities of a Nuclear Matter Created in Ultra Relativistic Nuclear Collisions
por: Kizka, V. A.
Publicado: (2015)
por: Kizka, V. A.
Publicado: (2015)
Constraints on Phase Transitions in Neutron Star Matter
por: Brandes, Len, et al.
Publicado: (2023)
por: Brandes, Len, et al.
Publicado: (2023)
Extended momentum-dependent interaction for transport models and neutron stars
por: Wang, Si-Pei, et al.
Publicado: (2025)
por: Wang, Si-Pei, et al.
Publicado: (2025)
Evidence for strong isovector nuclear spin-orbit interaction
por: Yue, Tong-Gang, et al.
Publicado: (2024)
por: Yue, Tong-Gang, et al.
Publicado: (2024)
Effects of isovector spin-orbit interaction on the charge-weak form factor difference in $^{48}$Ca, $^{208}$Pb, $^{90}$Zr and $^{62}$Ni
por: Yue, Tong-Gang, et al.
Publicado: (2026)
por: Yue, Tong-Gang, et al.
Publicado: (2026)
Extended Skyrme effective interactions with higher-order momentum-dependence for transport models and neutron stars
por: Wang, Si-Pei, et al.
Publicado: (2024)
por: Wang, Si-Pei, et al.
Publicado: (2024)
Anisotropic flows in Au+Au collisions at $\sqrt{s_{\rm{NN}}} = 2.4\,\text{GeV}$ with a Skyrme pseudopotential
por: Li, Xin, et al.
Publicado: (2025)
por: Li, Xin, et al.
Publicado: (2025)
Bayesian Inference of the Symmetry Energy and the Neutron Skin in $^{48}$Ca and $^{208}$Pb from CREX and PREX-2
por: Zhang, Zhen, et al.
Publicado: (2022)
por: Zhang, Zhen, et al.
Publicado: (2022)
Trace Anomaly of Cold Dense Matter Constrained by Collective Flow
por: Li, Bao-An
Publicado: (2026)
por: Li, Bao-An
Publicado: (2026)
Baryon density dependence of viscosities of the quark-gluon plasma at hadronization
por: Yang, Zhidong, et al.
Publicado: (2023)
por: Yang, Zhidong, et al.
Publicado: (2023)
Towards First Detection of the Solar MSW Transition With JUNO
por: Nairat, Obada, et al.
Publicado: (2025)
por: Nairat, Obada, et al.
Publicado: (2025)
Generalized relativistic second-order dissipative hydrodynamics: coupling different rank tensors
por: Harutyunyan, Arus, et al.
Publicado: (2025)
por: Harutyunyan, Arus, et al.
Publicado: (2025)
Critical slowing down and bulk viscosity in binary neutron star mergers
por: Karthein, Jamie M., et al.
Publicado: (2026)
por: Karthein, Jamie M., et al.
Publicado: (2026)
Non-Radial Oscillation Modes in Hybrid Stars with Hyperons and Delta Baryons
por: Rather, Ishfaq Ahmad, et al.
Publicado: (2024)
por: Rather, Ishfaq Ahmad, et al.
Publicado: (2024)
Axion-Like Particle Mediated Dark Matter and Neutron Star Properties in the QHD Model
por: Klangburam, Tanech, et al.
Publicado: (2025)
por: Klangburam, Tanech, et al.
Publicado: (2025)
Effect of Dark matter and $σ$-cut potential on radial and non-radial oscillation modes in neutron stars
por: Thakur, Prashant, et al.
Publicado: (2025)
por: Thakur, Prashant, et al.
Publicado: (2025)
Strangeon Matter: from Stars to Nuggets
por: Qi, Haoyang, et al.
Publicado: (2025)
por: Qi, Haoyang, et al.
Publicado: (2025)
Rotational enhancement and stability of protoquark stars during thermal evolution
por: Issifu, Adamu, et al.
Publicado: (2026)
por: Issifu, Adamu, et al.
Publicado: (2026)
Ejemplares similares
-
Pulsar as a Weber detector of gravitational waves and a probe to its internal phase transitions
por: Bagchi, Partha, et al.
Publicado: (2023) -
Pulse Modulation as a Signature of the Asteroid-Neutron Star Collision Model for High-Energy Transients
por: Bagchi, Partha, et al.
Publicado: (2026) -
Large-scale unpinning and pulsar glitches due to the forced oscillation of vortices
por: Layek, Biswanath, et al.
Publicado: (2024) -
Fastest spinning millisecond pulsars: indicators for quark matter in neutron stars?
por: Gärtlein, Christoph, et al.
Publicado: (2024) -
Orbital eccentricity can make neutron star g-mode resonances observable with current gravitational-wave detectors
por: Takátsy, János, et al.
Publicado: (2026)