1,971 research outputs found
A relative Hilbert-Mumford criterion
We generalize the classical Hilbert-Mumford criteria for GIT (semi-)stability
in terms of one parameter subgroups of a linearly reductive group G over a
field k, to the relative situation of an equivariant, projective morphism X ->
Spec A to a noetherian k-algebra A. We also extend the classical projectivity
result for GIT quotients: the induced morphism X^ss/G -> Spec A^G is
projective. As an example of applications to moduli problems, we consider
degenerations of Hilbert schemes of points.Comment: v4: minor correction
Speech Analysis
Contains research objectives and reports on one research project.National Science Foundatio
The COMPLETE Survey of Outflows in Perseus
We present a study on the impact of molecular outflows in the Perseus
molecular cloud complex using the COMPLETE survey large-scale 12CO(1-0) and
13CO(1-0) maps. We used three-dimensional isosurface models generated in
RA-DEC-Velocity space to visualize the maps. This rendering of the molecular
line data allowed for a rapid and efficient way to search for molecular
outflows over a large (~ 16 sq. deg.) area. Our outflow-searching technique
detected previously known molecular outflows as well as new candidate outflows.
Most of these new outflow-related high-velocity features lie in regions that
have been poorly studied before. These new outflow candidates more than double
the amount of outflow mass, momentum, and kinetic energy in the Perseus cloud
complex. Our results indicate that outflows have significant impact on the
environment immediately surrounding localized regions of active star formation,
but lack the energy needed to feed the observed turbulence in the entire
Perseus complex. This implies that other energy sources, in addition to
protostellar outflows, are responsible for turbulence on a global cloud scale
in Perseus. We studied the impact of outflows in six regions with active star
formation within Perseus of sizes in the range of 1 to 4 pc. We find that
outflows have enough power to maintain the turbulence in these regions and
enough momentum to disperse and unbind some mass from them. We found no
correlation between outflow strength and star formation efficiency for the six
different regions we studied, contrary to results of recent numerical
simulations. The low fraction of gas that potentially could be ejected due to
outflows suggests that additional mechanisms other than cloud dispersal by
outflows are needed to explain low star formation efficiencies in clusters.Comment: Published in The Astrophysical Journa
A GIT construction of degenerations of Hilbert schemes of points
We present a Geometric Invariant Theory (GIT) con-struction which allows us to construct good projective degenerationsof Hilbert schemes of points for simple degenerations. A comparisonwith the construction of Li and Wu shows that our GIT stack andthestack they construct are isomorphic, as are the associated coarse mod-uli schemes. Our construction is sufficiently explicit to obtain goodcontrol over the geometry of the singular fibres. We illustrate thisby giving a concrete description of degenerations of degreenHilbertschemes of a simple degeneration with two components
The geometry of degenerations of Hilbert schemes of points
Given a strict simple degeneration the first three authors
previously constructed a degeneration of the relative degree
Hilbert scheme of -dimensional subschemes. In this paper we investigate
the geometry of this degeneration, in particular when the fibre dimension of
is at most . In this case we show that is a dlt model.
This is even a good minimal dlt model if has this property.
We compute the dual complex of the central fibre and relate
this to the essential skeleton of the generic fibre. For a type II degeneration
of surfaces we show that the stack carries a
nowhere degenerate relative logarithmic -form. Finally we discuss the
relationship of our degeneration with the constructions of Nagai.Comment: 53 pages. To appear in J. Algebraic Geo
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