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- W3102969765 endingPage "103791" @default.
- W3102969765 startingPage "103791" @default.
- W3102969765 abstract "We construct a generalized EFT approach to dense compact-star matter that exploits the CCP for hadron-quark continuity at high density, hidden topology and hidden symmetries of QCD. No Landau-Ginzburg-Wilsonian-type phase transition is involved. The microscopic DoF of QCD possibly intervening at high baryonic density are traded in for fractionalized topological objects. Essential in the description are symmetries invisible in QCD in the matter-free vacuum: Scale symmetry, flavor local symmetry and parity-doubling. The partial emergence of scale symmetry is signaled by a dilatonic scalar in a pseudo-conformal structure. Flavor gauge symmetry manifests with the $rho$ meson mass going toward a Wilsonian RGFP identified with the VMFP at which the gauge boson mass goes to zero. Parity doubling is to take place as the quasi-nucleon mass converges to the chiral invariant $m_0$. The theory accounts satisfactorily for all known properties of normal nuclear matter and makes certain predictions that are drastically different from what's available in the literature. In particular, it provides a topological mechanism, argued to be robust, for the cross-over from soft-to-hard EoS that predicts the star properties in overall agreement with the presently available data, including the maximum star mass $M_{max}sim 2.3 M_odot$ and the recent LIGO/Virgo GW data. What is most glaringly different from all other approaches known, however, is the prediction for the rapid convergence to a sound velocity of star $v_s^2approx 1/3$ at a density $ngsim 3 n_0$, far from the asymptotic density $gsim 50n_0$ expected in pQCD. We interpret this to signal the onset of albeit approximate conformal symmetry in dense compact-star matter. The model developed here could bring out a new paradigm in nuclear/hadron physics, exploiting ideas in condensed matter physics, nuclear and particle physics and astrophysics." @default.
- W3102969765 created "2020-11-23" @default.
- W3102969765 creator A5070609280 @default.
- W3102969765 creator A5083834709 @default.
- W3102969765 date "2020-07-01" @default.
- W3102969765 modified "2023-10-05" @default.
- W3102969765 title "Towards the hadron–quark continuity via a topology change in compact stars" @default.
- W3102969765 cites W1907786740 @default.
- W3102969765 cites W1965461171 @default.
- W3102969765 cites W1971702030 @default.
- W3102969765 cites W1975963660 @default.
- W3102969765 cites W1978790589 @default.
- W3102969765 cites W1980799347 @default.
- W3102969765 cites W1982388729 @default.
- W3102969765 cites W1988305313 @default.
- W3102969765 cites W1991841581 @default.
- W3102969765 cites W2000304974 @default.
- W3102969765 cites W2008039793 @default.
- W3102969765 cites W2017672816 @default.
- W3102969765 cites W2018844967 @default.
- W3102969765 cites W2024294891 @default.
- W3102969765 cites W2034430164 @default.
- W3102969765 cites W2035407242 @default.
- W3102969765 cites W2037788066 @default.
- W3102969765 cites W2043368040 @default.
- W3102969765 cites W2043480920 @default.
- W3102969765 cites W2044127898 @default.
- W3102969765 cites W2046721419 @default.
- W3102969765 cites W2049984342 @default.
- W3102969765 cites W2056108655 @default.
- W3102969765 cites W2056470844 @default.
- W3102969765 cites W2061254829 @default.
- W3102969765 cites W2075227120 @default.
- W3102969765 cites W2076751616 @default.
- W3102969765 cites W2077293069 @default.
- W3102969765 cites W2077899510 @default.
- W3102969765 cites W2080311006 @default.
- W3102969765 cites W2082666420 @default.
- W3102969765 cites W2082719568 @default.
- W3102969765 cites W2092057151 @default.
- W3102969765 cites W2092350553 @default.
- W3102969765 cites W2094755808 @default.
- W3102969765 cites W2095971242 @default.
- W3102969765 cites W2107434716 @default.
- W3102969765 cites W2122160419 @default.
- W3102969765 cites W2124590498 @default.
- W3102969765 cites W2128398427 @default.
- W3102969765 cites W2134505714 @default.
- W3102969765 cites W2147590284 @default.
- W3102969765 cites W2165591715 @default.
- W3102969765 cites W2166885551 @default.
- W3102969765 cites W2167381994 @default.
- W3102969765 cites W2167572849 @default.
- W3102969765 cites W2278916484 @default.
- W3102969765 cites W2301645952 @default.
- W3102969765 cites W2519949689 @default.
- W3102969765 cites W2567411206 @default.
- W3102969765 cites W2768265440 @default.
- W3102969765 cites W2769916173 @default.
- W3102969765 cites W2775551765 @default.
- W3102969765 cites W2778488581 @default.
- W3102969765 cites W2795486177 @default.
- W3102969765 cites W2887055226 @default.
- W3102969765 cites W2896102426 @default.
- W3102969765 cites W2898610873 @default.
- W3102969765 cites W2898776745 @default.
- W3102969765 cites W2899521871 @default.
- W3102969765 cites W2903413419 @default.
- W3102969765 cites W2919003435 @default.
- W3102969765 cites W2953354871 @default.
- W3102969765 cites W2955406370 @default.
- W3102969765 cites W2963727897 @default.
- W3102969765 cites W2964623447 @default.
- W3102969765 cites W3037191297 @default.
- W3102969765 cites W3098281253 @default.
- W3102969765 cites W3099195819 @default.
- W3102969765 cites W3099651099 @default.
- W3102969765 cites W3100054390 @default.
- W3102969765 cites W3100060538 @default.
- W3102969765 cites W3100539265 @default.
- W3102969765 cites W3101529726 @default.
- W3102969765 cites W3101767342 @default.
- W3102969765 cites W3101892236 @default.
- W3102969765 cites W3102404673 @default.
- W3102969765 cites W3102458775 @default.
- W3102969765 cites W3102839133 @default.
- W3102969765 cites W3102952193 @default.
- W3102969765 cites W3103418798 @default.
- W3102969765 cites W3103657055 @default.
- W3102969765 cites W3104221123 @default.
- W3102969765 cites W3105006510 @default.
- W3102969765 cites W3105302986 @default.
- W3102969765 cites W3106358816 @default.
- W3102969765 cites W3106420367 @default.
- W3102969765 cites W4213182844 @default.
- W3102969765 cites W4232314582 @default.
- W3102969765 cites W4240130853 @default.
- W3102969765 cites W4293181570 @default.