2021
DOI: 10.3390/sym13101888
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Dichotomy of Baryons as Quantum Hall Droplets and Skyrmions: Topological Structure of Dense Matter

Abstract: We review a new development on the possible direct connection between the topological structure of the Nf=1 baryon as a FQH droplet and that of the Nf≥2 baryons (such as nucleons and hyperons) as skyrmions. This development suggests a possible “domain-wall (DW)” structure of compressed baryonic matter at high density expected to be found in the core of massive compact stars. Our theoretical framework is anchored on an effective nuclear effective field theory that incorporates two symmetries either hidden in th… Show more

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Cited by 12 publications
(19 citation statements)
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References 57 publications
(167 reference statements)
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“…As argued in [63], the FQH droplet should become relevant at some high density at which f χ → 0. This density must then be (much) higher than that reached at the DLFP close to the GD's IR fixed point.…”
Section: Indispensable Role Of Vector Mesonsmentioning
confidence: 82%
See 2 more Smart Citations
“…As argued in [63], the FQH droplet should become relevant at some high density at which f χ → 0. This density must then be (much) higher than that reached at the DLFP close to the GD's IR fixed point.…”
Section: Indispensable Role Of Vector Mesonsmentioning
confidence: 82%
“…There are two questions raised regarding this dichotomy [63] between the skyrmions and the FQH droplets. The first is: is there any relation between the two topological objects, the FQH droplet for B (0) and the skyrmion for nucleons?…”
Section: No Infinite Hotel For N F = 1 Baryonsmentioning
confidence: 99%
See 1 more Smart Citation
“…Dense nuclear matter relevant to the core of compact star is an uncharted domain although it has been studied for several decades [1][2][3][4][5][6][7][8]. Several fundamental but significant questions in dense nuclear matter, such as the pattern of symmetry, the constituents and so on are not yet well understood.…”
Section: Introductionmentioning
confidence: 99%
“…Several fundamental but significant questions in dense nuclear matter, such as the pattern of symmetry, the constituents and so on are not yet well understood. The recent observations of massive neutron stars with about two times solar mass and detections of the gravitational waves from binary neutron star mergers and neutron star-black hole mergers open new laboratories for dense nuclear matter (see, e.g., [5][6][7][8] and references therein).…”
Section: Introductionmentioning
confidence: 99%