collapse

The Evolution of a Financial Crisis:

Collapse of the Asset-Backed Commercial Paper Market*

DANIEL COVITZ, NELLIE LIANG, and GUSTAVO A. SUAREZ

April 5, 2012

ABSTRACT

This paper documents “runs” on asset-backed commercial paper (ABCP) programs using a novel dataset of all transactions in the U.S. market during its severe contraction in 2007. We find that one-third of programs were run within weeks of the onset of the ABCP crisis and that runs, as well as yields and maturities for new issues, were related to program-level and macr

Critical collapse of a self-gravitating scalar field in a (2+1)-dimensional spacetime with negative cosmological constant seems to be dominated by a continuously self-similar solution of the field equations without cosmological constant. However, previous

Critical collapse of a self-gravitating scalar field in a (2+1)-dimensional spacetime with negative cosmological constant seems to be dominated by a continuously self-similar solution of the field equations without cosmological constant. However, previous

Critical collapse o

We present a general framework to treat the evolution of one-point probability distribution function (PDF) for cosmic density $\delta$ and velocity-divergence fields $\theta$. In particular, we derive an evolution equation for the one-point PDFs and consid

RESCEU-18/02UTAP-429/2002

EvolutionofCosmologicalDensityDistributionFunctionfromthe

LocalCollapseModel

YasuhiroOhta,IsshaKayoandAtsushiTaruya

arXiv:astro-ph/0301567v1 29 Jan 2003DepartmentofPhysicsandResearchCenterfortheEarlyUniverse(RESCEU),SchoolofScience,UniversityofTokyo,

We present a general framework to treat the evolution of one-point probability distribution function (PDF) for cosmic density $\delta$ and velocity-divergence fields $\theta$. In particular, we derive an evolution equation for the one-point PDFs and consid

RESCEU-18/02UTAP-429/2002

EvolutionofCosmologicalDensityDistributionFunctionfromthe

LocalCollapseModel

YasuhiroOhta,IsshaKayoandAtsushiTaruya

arXiv:astro-ph/0301567v1 29 Jan 2003DepartmentofPhysicsandResearchCenterfortheEarlyUniverse(RESCEU),SchoolofScience,UniversityofTokyo,

Gravitational collapse in (n+2) dimensional quasi-spherical space-time is studied for a fluid with non vanishing radial pressure. An exact analytic solution is obtained (ignoring the arbitrary integration function) for the equation of state $p_{r}=(\gamma-

Gravitational collapse in (n+2) dimensional quasi-spherical space-time is studied for a fluid with non vanishing radial pressure. An exact analytic solution is obtained (ignoring the arbitrary integration function) for the equation of state $p_{r}=(\gamma-

Gravitational col

We give a model of the higher-dimensional spherically symmetric gravitational collapse of a dust cloud in Einstein-Gauss-Bonnet gravity. A simple formulation of the basic equations is given for the spacetime $M \approx M^2 \times K^{n-2}$ with a perfect fl

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aFinalfateofsphericallysymmetricgravitationalcollapseofadustcloudinEinstein-Gauss-BonnetgravityHidekiMaeda AdvancedResearchInstituteforScienceandEngineering,WasedaUniversity,Okubo3-4-1,Shinjuku,Tokyo169-8555,Japan(Dated:February7,2008)Wegiveamodelof