activity
20042026
most citedSignatures of hadron-quark mixed phase in gravitational waves

150 citations · 981 across the 54 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

7 papers · 1 filter

astro-ph.SR2022★ 1 cited

A Lagrangian construction of rotating stars

Misa Ogata, Hirotada Okawa, Kotaro Fujisawa +3

We present a new formulation for numerically obtaining axisymmetric equilibrium structures of rotating stars in two spatial dimensions. With a view to apply it to the secular evolu…

astro-ph.SR2015

Cooling of Compact Stars with Color Superconducting Quark Matter

Tsuneo Noda, Nobutoshi Yasutake, Masa-aki Hashimoto +3

We show a scenario for the cooling of compact stars considering the central source of Cassiopeia A (Cas A). The Cas A observation shows that the central source is a compact star wi…

astro-ph.SR2014★ 8 cited

A Novel Formulation by Lagrangian Variational Principle for Rotational Equilibria: Toward Multi-Dimensional Stellar Evolutions

Nobutoshi Yasutake, Kotaro Fujisawa, Shoichi Yamada

We have developed a new formulation to obtain self-gravitating, axisymmetric configurations in permanent rotation. The formulation is based on the Lagrangian variational principle,…

astro-ph.SR2013★ 25 cited

Structure of the hadron-quark mixed phase in protoneutron stars

H. Chen, G. F. Burgio, H. -J. Schulze +1

We study the hadron-quark phase transition in the interior of hot protoneutron stars, combining the Brueckner-Hartree-Fock approach for hadronic matter with the MIT bag model or th…

astro-ph.SR2013★ 11 cited

Rapid Spin Deceleration of Magnetized Proto-Neutron Stars via Asymmetric Neutrino Emission

T. Maruyama, J. Hidaka, T. Kajino +5

We calculate the spin deceleration of proto-neutron stars by asymmetric neutrino absorption in the context of a fully relativistic mean field theory. We calculate for the first tim…

astro-ph.SR2011★ 48 cited

Cooling of Compact Stars with Color Superconducting Phase in Quark Hadron Mixed Phase

Tsuneo Noda, Masa-aki Hashimoto, Nobutoshi Yasutake +3

We present a new scenario for the cooling of compact stars considering the central source of Cassiopeia A (Cas A). The Cas A observation shows that the central source is a compact…