activity
20112023
most citedThermodynamic consistency, quark mass scaling, and properties of strange matter

88 citations · 796 across the 33 of their papers we have counts for

collaborators
Showing 2022Show all

8 papers · 1 filter

astro-ph.HE2022★ 18 cited

Probing phase transition in neutron stars via the crust-core interfacial mode

Jiaxiang Zhu, Chuming Wang, Chengjun Xia +2

Gravitational waves emitted from the binary neutron star (BNS) systems can carry information about the dense matter phase in these compact stars. The crust-core interfacial mode is…

hep-ph2022★ 16 cited

Bulk Strong Matter: the Trinity

Xiaoyu Lai, Chengjun Xia, Renxin Xu

Our world is wonderful because of the normal but negligibly small baryonic part (i.e., atoms) although unknown dark matter and dark energy dominate the Universe. A stable atomic nu…

nucl-th2022★ 8 cited

Elastic properties of nuclear pasta in a fully three-dimensional geometry

Cheng-Jun Xia, Toshiki Maruyama, Nobutoshi Yasutake +2

Realistic estimations on the elastic properties of neutron star matter are carried out with a large strain () in the framework of relativistic-mean-field…

nucl-th2022★ 42 cited

Unified neutron star EOSs and neutron star structures in RMF models

Cheng-Jun Xia, Toshiki Maruyama, Ang Li +3

In the framework of Thomas-Fermi approximation, we study systematically the EOSs and microscopic structures of neutron star matter in a vast density range with $n_\mathrm{b}\approx…

nucl-th2022★ 6 cited

Nuclear pasta structures at high temperatures

Cheng-Jun Xia, Toshiki Maruyama, Nobutoshi Yasutake +1

We investigate nuclear pasta structures at high temperatures in the framework of relativistic mean field model with Thomas-Fermi approximation. Typical pasta structures (droplet, r…

hep-ph2022

Deconfinement phase transition and quark condensate in compact stars

Hao-Miao Jin, Cheng-Jun Xia, Ting-Ting Sun +1

We investigate systematically the possible deconfinement phase transition from nuclear matter to quark matter in compact stars. The properties of nuclear matter are fixed by expand…