Armen Sedrakian

Professor UWr

Wroclaw University of Science and Technology

Poland

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Professor Armen Sedrakian is a faculty member at Wroclaw University in Poland. His research primarily focuses on astrophysics, with recent articles exploring topics such as dissipative hydrodynamics, the properties of rapidly rotating neutron stars, and Bayesian inferences on covariant density functionals. Additionally, he investigates superconductivity in magnetars and various phenomena associated with neutron stars and dense electron-ion plasma.

Articles (27)

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Collaborators (4)

David Blaschke

Professor

University of Wrocław

POLAND

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Mateusz Cierniak

University of Wrocław

POLAND

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Jiajie Li

GERMANY

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David Edwin Alvarez-Castillo

Assistant Professor

Institute of Nuclear Physics Polish Academy of Sciences

POLAND

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Armen Sedrakian

Research Interests

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About

Articles (27)

Effect of symmetry energy on properties of rapidly rotating neutron stars and universal relations

Bayesian inferences on covariant density functionals from multimessenger astrophysical data: The impacts of likelihood functions of low density matter constraints

Bayesian constraints on covariant density functional equations of state of compact stars with new NICER mass-radius measurements

Bayesian inferences on covariant density functionals from multimessenger astrophysical data: Nucleonic models

Confronting new NICER mass-radius measurements with phase transition in dense matter and twin compact stars

Generalized relativistic second-order dissipative hydrodynamics: Coupling different rank tensors

Superconductivity in magnetars: Exploring type-I and type-II states in toroidal magnetic fields

Josephson currents in neutron stars

Bulk viscosity of two-color superconducting quark matter in neutron star mergers

Extremely small stars in scalar-tensor gravity: When stellar radius is less than Schwarzschild one

Finite-temperature equations of state of compact stars with hyperons: three-dimensional tables

Hybrid Star Models in the Light of New Multimessenger Data

Electrical conductivity of a warm neutron star crust in magnetic fields: Neutron-drip regime

Thermal Conductivity and Thermal Hall Effect in Dense Electron-Ion Plasma

Short-Range Correlations and Urca Process in Neutron Stars

Universal relations for compact stars with heavy baryons

Impact of Multiple Phase Transitions in Dense QCD on Compact Stars

Heavy baryons in compact stars

Two first-order phase transitions in hybrid compact stars: Higher-order multiplet stars, reaction modes, and intermediate conversion speeds

Phenomenological Relativistic Second-Order Hydrodynamics for Multiflavor Fluids

Relativistic Hybrid Stars with Sequential First-order Phase Transitions in Light of Multimessenger Constraints

Ultracompact hybrid stars consistent with multimessenger astrophysics

New Covariant Density Functionals of Nuclear Matter for Compact Star Simulations

Bulk viscosity from Urca processes: npeμ matter in the neutrino-transparent regime

Universal relations for rapidly rotating cold and hot hybrid stars

Bulk Viscosity of Relativistic npeμ Matter in Neutron-Star Mergers

Delta-resonances and hyperons in proto-neutron stars and merger remnants

Collaborators (4)

David Blaschke

Mateusz Cierniak

Jiajie Li

David Edwin Alvarez-Castillo

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