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Thermal and electric conductivities of relativistic degenerate electrons are calculated for the case when electrons scatter by phonons in Coulomb crystals made of spherical finite--size nuclei at densities $10^{11}$~g/cm$^3 < \rho <…

Astrophysics · Physics 2007-05-23 D. A. Baiko , D. G. Yakovlev

It is believed that quark stars or neutron stars with mixed phase in the core have smaller radii compared to ordinary compact stars. With the recent observation of several low radius objects, typically a radius of $<10 Km.$ for star of mass…

High Energy Physics - Phenomenology · Physics 2009-11-10 Ashok Goyal

The polaron binding energy E_{p} in undoped parent cuprates has been determined to be about 1.0 eV from the unconventional oxygen-isotope effect on the antiferromagnetic ordering temperature. The deduced value of E_{p} is in quantitative…

Superconductivity · Physics 2009-11-10 Guo-meng Zhao

The matter inside pulsar-like compact stars could be in a quark-cluster phase since in cold dense matter at a few nuclear densities (2 to 10 times), quarks could be coupled still very strongly and condensate in position space to form quark…

High Energy Astrophysical Phenomena · Physics 2015-06-03 Shi Dai , Renxin Xu

We investigate the influence of a phase transition from hadronic matter to a deconfined quark phase inside a neutron star on its cooling behaviour including the appearance of twin star solutions in the mass-radius diagram. We find that…

High Energy Astrophysical Phenomena · Physics 2025-02-21 Melissa Mendes , Jan-Erik Christian , Farrukh J. Fattoyev , Jürgen Schaffner-Bielich

Bose condensed light can form new phases [1] in a dye filled cavity due to the presence of the orientational disorder created by dye molecules which are essentially frozen on the time scale of the photonic thermalization (few ps). At longer…

Quantum Gases · Physics 2020-05-06 Victor Fleurov , Anatoly B. Kuklov

We study the thermal evolution of neutron stars containing deconfined quark matter in their core. Such objects are generally referred to as quark-hybrid stars. The confined hadronic matter in their core is described in the framework of…

Nuclear Theory · Physics 2016-01-13 S. M. de Carvalho , R. Negreiros , M. Orsaria , G. A. Contrera , F. Weber , W. Spinella

Separating electron and phonon thermal conductivity components is imperative for understanding the principle thermal transport mechanisms in metals and highly desirable in many applications. In this work, we predict the mode-dependent…

Materials Science · Physics 2019-10-23 Zhen Tong , Shouhang Li , Xiulin Ruan , Hua Bao

Reflectivity as a function of temperature for the La$_{0.67}$Ca$_{0.33}$MnO$_{3}$ (LCMO) film has been measured across the metal-insulator phase transition. The optical properties and their temperature dependence were determined in the…

Strongly Correlated Electrons · Physics 2018-04-02 Naween Anand , Naveen Margankunte , Hyoungjeen Jeen , A. F. Hebard , Amlan Biswas , David B. Tanner

We study a spin-1 single flavor color superconducting phase which results from a color-spin locking (CSL) interaction in two-flavor quark matter. This phase is particularly interesting for compact star cooling applications since the CSL…

High Energy Physics - Phenomenology · Physics 2009-11-11 D. N. Aguilera , D. Blaschke , M. Buballa , V. L. Yudichev

Solar flares effectively accelerate particles to non-thermal energies. These accelerated electrons are responsible for energy transport and subsequent emissions in HXR, radio, and UV/EUV radiation. Due to the steeply decreasing electron…

Solar and Stellar Astrophysics · Physics 2026-01-01 Yingjie Luo , Eduard P. Kontar , Debesh Bhattacharjee

By studying the temperature-dependent behavior of electron thermal conductivity (k) in a 3.2 nm-thin film, we quantify the extremely confined defect-electron scattering and reveal the intrinsic phonon-electron scattering that is shared by…

Mesoscale and Nanoscale Physics · Physics 2015-01-16 Zhe Cheng , Zaoli Xu , Shen Xu , Xinwei Wang

The core of neutron-star matter is supposed to be at a much higher density than the normal nuclear matter density for which various possibilities have been suggested such as, for example, meson or hyperon condensation and/or deconfined…

High Energy Astrophysical Phenomena · Physics 2011-10-07 Kyungmin Kim , Hyun Kyu Lee , Mannque Rho

Some isolated neutron stars show harmonically spaced absorption features in their thermal soft X-ray spectra. The interpretation of the features as a cyclotron line and its harmonics has been suggested, but the usual explanation of the…

High Energy Astrophysical Phenomena · Physics 2015-05-14 V. F. Suleimanov , G. G. Pavlov , K. Werner

We compute the thermal conductivity and thermoelectric power (thermopower) of the inner crust of compact stars across a broad temperature-density domain relevant for proto-neutron stars, binary neutron-star mergers, and accreting neutron…

High Energy Astrophysical Phenomena · Physics 2025-12-02 Henrik Danielyan , Arus Harutyunyan , Armen Sedrakian

Baryon and quark superfluidity in the cooling of neutron stars are investigated. Observations could constrain combinations of the neutron or Lambda-hyperon pairing gaps and the star's mass. However, in a hybrid star with a mixed phase of…

High Energy Physics - Phenomenology · Physics 2011-05-05 Dany Page , Madappa Prakash , James M. Lattimer , Andrew Steiner

Spin-one color superconductor is a viable candidate phase of dense matter in the interiors of compact stars. Its low-energy excitations will influence the transport properties of such matter and thus have impact on late-stage evolution of…

High Energy Physics - Phenomenology · Physics 2014-11-20 Tomas Brauner , Jin-yi Pang , Qun Wang

The hopping of an electron, interacting with many ions of a lattice via the long-range (Fr\"{o}hlich) electron-phonon interaction and optical absorption are studied at zero temperature. Ions are assumed to be isotropic three-dimensional…

Quantum Physics · Physics 2007-05-23 B. Ya. Yavidov

For the intrinsic carriers of MAPbBr$_{3}$, the temperature $T$ dependent mobility $\mu(T)$ of behaves like $\mu\propto T^{-1/2}$ in piezoelectric tetragonal phase, $\mu\propto T^{-1.4}$ in non-piezoelectric cubic phase. But for the…

Materials Science · Physics 2018-05-07 Ming-Hui Zhang , Ming-Liang Zhang

We study the deconfinement transition of hadronic matter into quark matter under neutron star conditions assuming color and flavor conservation during the transition. We use a two-phase description. For the hadronic phase we use different…

High Energy Astrophysical Phenomena · Physics 2009-09-02 G. Lugones , A. G. Grunfeld , N. N. Scoccola , C. Villavicencio