6,716 research outputs found
Ratio coordinates for higher Teichm\"uller spaces
We define new coordinates for Fock-Goncharov's higher Teichm\"uller spaces
for a surface with holes, which are the moduli spaces of representations of the
fundamental group into a reductive Lie group . Some additional data on the
boundary leads to two closely related moduli spaces, the -space
and the -space, forming a cluster ensemble. Fock and Goncharov
gave nice descriptions of the coordinates of these spaces in the cases of and , together with Poisson structures. We consider new
coordinates for higher Teichm\"uller spaces given as ratios of the coordinates
of the -space for , which are generalizations of Kashaev's
ratio coordinates in the case . Using Kashaev's quantization for , we
suggest a quantization of the system of these new ratio coordinates, which may
lead to a new family of projective representations of mapping class groups.
These ratio coordinates depend on the choice of an ideal triangulation
decorated with a distinguished corner at each triangle, and the key point of
the quantization is to guarantee certain consistency under a change of such
choices. We prove this consistency for , and for completeness we also give
a full proof of the presentation of Kashaev's groupoid of decorated ideal
triangulations.Comment: 42 pages, 6 figure
The dilogarithmic central extension of the Ptolemy-Thompson group via the Kashaev quantization
Quantization of universal Teichm\"uller space provides projective
representations of the Ptolemy-Thompson group, which is isomorphic to the
Thompson group . This yields certain central extensions of by
, called dilogarithmic central extensions. We compute a
presentation of the dilogarithmic central extension of
resulting from the Kashaev quantization, and show that it corresponds to
times the Euler class in . Meanwhile, the braided
Ptolemy-Thompson groups , of Funar-Kapoudjian are extensions of
by the infinite braid group , and by abelianizing the kernel
one constructs central extensions , of
by , which are of topological nature. We show . Our result is analogous to that of Funar and Sergiescu, who
computed a presentation of another dilogarithmic central extension
of resulting from the Chekhov-Fock(-Goncharov) quantization
and thus showed that it corresponds to times the Euler class and that
. In addition, we suggest a natural relationship
between the two quantizations in the level of projective representations.Comment: 43 pages, 15 figures. v2: substantially revised from the first
version, and the author affiliation changed. // v3: Groups M and T are shown
to be anti-isomorphic (new Prop.2.32), which makes the whole construction
more natural. And some minor changes // v4: reflects all changes made for
journal publication (to appear in Adv. Math.
Topology Change and Tensor Forces for the EoS of Dense Baryonic Matter
When skyrmions representing nucleons are put on crystal lattice and
compressed to simulate high density, there is a transition above the normal
nuclear matter density from a matter consisting of skyrmions with integer
baryon charge to a state of half-skyrmions with half-integer baryon charge. We
exploit this observation in an effective field theory formalism to access dense
baryonic system. We find that the topology change involved implies a changeover
from a Fermi liquid structure to a non-Fermi liquid with the chiral condensate
in the nucleon "melted off." The of the nucleon mass that remains,
invariant under chiral transformation, points to the origin of the (bulk of)
proton mass that is not encoded in the standard mechanism of spontaneously
broken chiral symmetry. The topology change engenders a drastic modification of
the nuclear tensor forces, thereby nontrivially affecting the EoS, in
particular, the symmetry energy, for compact star matter. It brings in
stiffening of the EoS needed to accommodate a neutron star of solar
mass. The strong effect on the EoS in general and in the tensor force structure
in particular will also have impact on processes that could be measured at
RIB-type accelerators.Comment: 16 pages, 4 figures: Note dedicated to Gerry Brown, prepared for
contribution to "EPJA Special Volume on Nuclear Symmetry Energy.
Nuclear Symmetry Energy with Strangeness in Heavy Ion Collision
The role of anti-kaons in the symmetry energy to be determined in heavy-ion
collisions as for instance in such observables as the ratio is
discussed using a simple chiral Lagrangian. It is shown, with some mild
assumptions, that kaons, when present in the system, can affect the EoS
appreciably for both symmetric and asymmetric nuclear matter. For nuclear
matter with small asymmetry with which heavy-ion collisions are studied, it may
be difficult to distinguish a stiff symmetry energy and the supersoft symmetry
energy, even with kaons present. However the effect of kaon is found to be
significant such that near , at which the chemical
potential difference is zero without kaon amplitude. We present the argument
that in order to obtain a reliably accurate equation of state (EoS) for
compact-star matter, a much deeper understanding is needed on how the
strangeness degrees of freedom such as kaons, hyperons etc. behave in baryonic
matter in a Fermi liquid (or possibly a non-Fermi liquid) phase with potential
phase changes. It is suggested that such an {\em accurate} treatment could have
an important implication on possibly modified gravity.Comment: 13 pages, 3 figures. revised for publicatio
Dilatons in Dense Baryonic Matter
We discuss the role of dilaton, which is supposed to be representing a
special feature of scale symmetry of QCD, trace anomaly, in dense baryonic
matter. The idea that the scale symmetry breaking of QCD is responsible for the
spontaneous breaking of chiral symmetry is presented along the similar spirit
of Freund-Nambu model. The incorporation of dilaton field in the hidden local
symmetric parity doublet model is briefly sketched with the possible role of
dilaton at high density baryonic matter, the emergence of linear sigma model in
dilaton limit.Comment: 7 pages, no figure
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