论文标题
致密的重质物质中的分数化准颗粒
Fractionalized Quasiparticles in Dense Baryonic Matter
论文作者
论文摘要
我讨论了一个新的方案，以了解如何将重磅液体变成由紧凑型恒星内部的高密度驱动的分数化的液体的费米液体。它涉及“隐藏”本地矢量bosons $ρ$和$ω$，以及“隐藏”的比例对称性diLaton $χ$，在Quark $ \ leftrightArrow $ Hadron duality和QCD的意义上都被视为QCD的“双重”，并提供了一个可能的cat式cat catsons''chessire tilly''天空和分数量子厅（FQH）液滴{\ it and}探索，随着密度超出正常核物质密度的密度，可以推定“解污”夸克的密度，以探讨重型物质的行为。关于“物质”的分数特征（无论它们是什么）是否可以在紧凑型恒星的致密恒星核心中“探测”，提出了一个问题。
I discuss a novel scenario on how baryonic matter could turn into a Fermi liquid of fractionalized baryons driven by high density inside compact stars. It involves the "hidden" local vector bosons $ρ$ and $ω$ together with the "hidden" scale symmetry dilaton $χ$, both taken to be "dual" to the quarks and gluons of QCD in the sense of quark $\leftrightarrow$ hadron duality and offers a possibility, exploiting the "Cheshire Cat Principle", to unify the "dichotomy" of baryons described in terms of skyrmions and fractional quantum Hall (FQH) droplets {\it and} to explore how the baryonic matter could behave as density goes way beyond the normal nuclear matter density to the density regime where "deconfined" quarks are presumed to figure. The question is raised as to whether the fractionalized characteristics of the "stuff" -- whatever they are -- can be "probed" in the dense star core of compact stars.
