8,423 research outputs found
Quantum traces for : the case
We generalize Bonahon and Wong's -quantum trace
map to the setting of . More precisely, for each
non-zero complex number , we associate to every isotopy class of framed
oriented links in a thickened punctured surface a Laurent polynomial in -deformations of the
Fock-Goncharov coordinates for a higher Teichm\"{u}ller space, depending
on the choice of an ideal triangulation of the surface
. Along the way, we propose a definition for a
-version of this invariant.Comment: 34 pages, 23 figures + 1 appendix; 48 pages in tota
Tropical Fock-Goncharov coordinates for -webs on surfaces II: naturality
In a companion paper (arXiv 2011.01768) we constructed non-negative integer
coordinates for a distinguished collection of -webs on a finite-type punctured surface
, depending on an ideal triangulation of
. We prove that these coordinates are natural with respect to the
choice of triangulation, in the sense that if a different triangulation
is chosen then the coordinate change map relating
and is a prescribed tropical
cluster transformation. Moreover, when is an ideal square,
we provide a topological geometric description of the Hilbert basis (in the
sense of linear programming) of the non-negative integer cone
, and
we prove that this cone canonically decomposes into 42 sectors corresponding
topologically to 42 families of -webs in the square.Comment: 39 pages, 27 figure
The Five Planets in the Kepler-296 Binary System All Orbit the Primary: A Statistical and Analytical Analysis
Kepler-296 is a binary star system with two M-dwarf components separated by
0.2 arcsec. Five transiting planets have been confirmed to be associated with
the Kepler-296 system; given the evidence to date, however, the planets could
in principle orbit either star. This ambiguity has made it difficult to
constrain both the orbital and physical properties of the planets. Using both
statistical and analytical arguments, this paper shows that all five planets
are highly likely to orbit the primary star in this system. We performed a
Markov-Chain Monte Carlo simulation using a five transiting planet model,
leaving the stellar density and dilution with uniform priors. Using importance
sampling, we compared the model probabilities under the priors of the planets
orbiting either the brighter or the fainter component of the binary. A model
where the planets orbit the brighter component, Kepler-296A, is strongly
preferred by the data. Combined with our assertion that all five planets orbit
the same star, the two outer planets in the system, Kepler-296 Ae and
Kepler-296 Af, have radii of 1.53 +/- 0.26 and 1.80 +/- 0.31 R_earth,
respectively, and receive incident stellar fluxes of 1.40 +/- 0.23 and 0.62 +/-
0.10 times the incident flux the Earth receives from the Sun. This level of
irradiation places both planets within or close to the circumstellar habitable
zone of their parent star.Comment: Accepted for publication in Ap
Do Electrostatic Interactions with Positively Charged Active Site Groups Tighten the Transition State for Enzymatic Phosphoryl Transfer?
The effect of electrostatic interactions on the transition-state character for enzymatic phosphoryl transfer has been a subject of much debate. In this work, we investigate the transition state for alkaline phosphatase (AP) using linear free-energy relationships (LFERs). We determined kcat/KM for a series of aryl sulfate ester monoanions to obtain the Brønsted coefficient, βlg, and compared the value to that obtained previously for a series of aryl phosphorothioate ester dianion substrates. Despite the difference in substrate charge, the observed Brønsted coefficients for AP-catalyzed aryl sulfate and aryl phosphorothioate hydrolysis (−0.76 ± 0.14 and −0.77 ± 0.10, respectively) are strikingly similar, with steric effects being responsible for the uncertainties in these values. Aryl sulfates and aryl phosphates react via similar loose transition states in solution. These observations suggest an apparent equivalency of the transition states for phosphorothioate and sulfate hydrolysis reactions at the AP active site and, thus, negligible effects of active site electrostatic interactions on charge distribution in the transition state
Electric utilities, fuel use, and responsiveness to fuel prices
This research tests the impact of changes in fuel price to explain fuel use by electric utilities. We employ a three-stage least squares model that explains changes in fuel use as a function of changes in three fuel prices. This model is repeated across sub-samples of data aggregated at the plant level and operating holding company level. We expect that plants and holding companies reduce fuel use when fuel prices rise. Several fuel substitution effects within and across plants and holding companies are demonstrated, as well as several frictions. At the plant level, higher prices of natural gas lead to less natural gas consumption, less coal consumption, and more fuel oil consumption. At the operating holding company level, results demonstrate the inelasticity of coal use and the increases of natural gas in response to higher coal prices. Subsamples demonstrate heterogeneity of results across different plants. Results emphasize that technological, market, and regulatory frictions may hinder the performance of energy policies
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