English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Tools annual

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools monthly

Global: Zendy Plus monthly

Presents the access of premium content as premium feature

Premium Content

Global: Zendy Plus annual

Global: Zendy Free Plan

Starting from equations of state of nucleonic and color-superconducting quarkmatter and assuming a first-order phase transition between these, we constructan equation of state of stellar matter, which contains three phases: anucleonic phase, as well as two-flavor and three-flavor color-superconductingphases of quarks. Static sequences of the corresponding hybrid stars includemassive members with masses of $\sim 2 M_{\odot}$ and radii in the range of$13< R < 16$ km. We investigate the integral parameters of rapidly rotatingstars and obtain evolutionary sequences that correspond to constant rest-massstars spinning down by electromagnetic and gravitational radiation. Physicallynew transitional sequences are revealed that are distinguished by a phasetransition from nucleonic to color-superconducting matter for someconfigurations that are located between the static and Keplerian limits. Thesnapshots of internal structure of the star, displaying the growth or shrinkageof superconducting volume as the star's spin changes, are displayed forconstant rest mass stars. We further obtain evolutionary sequences of rotatingsupramassive compact stars and construct pre-collapse models that can be usedas initial data to simulate a collapse of color-superconducting hybrid stars toa black hole.

Rotating hybrid compact stars