Conveners
Session 7
- Masayasu Harada (Nagoya Ubiversity)
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Prashant Thakur (Yonsei University)01/05/2026, 15:50
Abstract: Neutron stars provide a high-density laboratory to test dark matter (DM) through its gravitational imprint on stellar structure and early evolution. In this talk, I present a unified set of results based on two-fluid modeling of cold neutron stars and evolving proto-neutron stars (PNSs), together with Bayesian model selection, multi-messenger constraints, and inverse parameter...
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Yeunhwan Lim (Yonsei University)01/05/2026, 16:25
We study how the nuclear symmetry energy and its density slope parameter affect the neutron dripline of finite nuclei and the macroscopic properties of neutron stars within a semiclassical liquid drop model (LDM). Our analysis employs energy density functionals constrained by chiral effective field theory. The symmetry energy at saturation density is fixed, while the surface tension parameter...
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LIU Xiang01/05/2026, 17:00
This work focuses on the existence of pion condensate in neutron star matter based on a parity doublet model. Parity doublet model is a model that explains the hadron mass as two parts: one part is generated by spontaneous breaking of chiral symmetry and the other is an invariant mass that does not depend on the breaking of chiral symmetry and is called a chiral invariant mass $m_0$. A pion...
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Vivek Baruah Thapa (Birangana Sati Sadhani Rajyik Vishwavidyalaya)01/05/2026, 17:20
We present a unified Bayesian analysis of the dense-matter equation of state (EOS) of neutron stars by incorporating exotic hadronic degrees of freedom, namely antikaon condensation and Δ-resonances, within a density-dependent relativistic hadron framework. The model is constrained using nuclear saturation properties, chiral effective field theory ($\chi$EFT) calculations for symmetric and...
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Hao-Song You (Tsung-Dao Lee Institute, Shanghai Jiao Tong University)01/05/2026, 17:40
Using an equivparticle model with mean-field approximation (MFA), we systematically investigate quark matter properties across scales, from microscopic multibaryon states to macroscopic compact dwarfs. First, we determine the mass spectra of color-singlet $N$-quark configurations ($N=3$ to $18$) based on SU(6) symmetry and Bayesian inference. Our results predict several bound states, including...
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