The essential spectrum of Neumann Laplacians on some bounded singular domains
… be the set of all functions in L*(Q) whose distributional gradients are in L, and we define -A:
via … (0, L) x (0, w) of fixed length L and width w 6 L, with two adjoining rectangles S, and S, of …
via … (0, L) x (0, w) of fixed length L and width w 6 L, with two adjoining rectangles S, and S, of …
[PDF][PDF] On the energy of a large atom
CL Fefferman, LA Seco - 1990 - community.ams.org
We announce a proof of an asymptotic formula for the groundstate energy of a large atom.
The early work of Thomas-Fermi, Hartree-Fock, Dirac, and Scott predicted that for an atomic …
The early work of Thomas-Fermi, Hartree-Fock, Dirac, and Scott predicted that for an atomic …
The electromagnetic counterpart of the binary neutron star merger LIGO/Virgo GW170817. II. UV, optical, and near-infrared light curves and comparison to kilonova …
…, M Sauseda, DJ Schlegel, LF Secco… - The Astrophysical …, 2017 - iopscience.iop.org
We present UV, optical, and near-infrared (NIR) photometry of the first electromagnetic
counterpart to a gravitational wave source from Advanced Laser Interferometer Gravitational-…
counterpart to a gravitational wave source from Advanced Laser Interferometer Gravitational-…
Dark Energy Survey Year 1 results: Cosmological constraints from cosmic shear
We use 26× 10 6 galaxies from the Dark Energy Survey (DES) Year 1 shape catalogs over
1321 deg 2 of the sky to produce the most significant measurement of cosmic shear in a …
1321 deg 2 of the sky to produce the most significant measurement of cosmic shear in a …
Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and weak lensing
We present the first cosmology results from large-scale structure using the full 5000 deg 2 of
imaging data from the Dark Energy Survey (DES) Data Release 1. We perform an analysis …
imaging data from the Dark Energy Survey (DES) Data Release 1. We perform an analysis …
Living in a world of our own: The experience of parents who have a child with autism
RL Woodgate, C Ateah, L Secco - Qualitative health …, 2008 - journals.sagepub.com
In this article, we discuss findings of a hermeneutic phenomenological study that sought to
describe the experiences of parents who have a child with autism. Qualitative interviews were …
describe the experiences of parents who have a child with autism. Qualitative interviews were …
Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to data calibration
… The lightcones are run with the LGADGET2 N-body code, a memory optimized version of
GADGET2 [… in terms of the convergence power spectrum Cκ(l) at an angular wave number l as …
GADGET2 [… in terms of the convergence power spectrum Cκ(l) at an angular wave number l as …
The electromagnetic counterpart of the binary neutron star merger LIGO/Virgo GW170817. I. Discovery of the optical counterpart using the dark energy camera
…, M Sauseda, DJ Schlegel, LF Secco… - The Astrophysical …, 2017 - iopscience.iop.org
We present the Dark Energy Camera (DECam) discovery of the optical counterpart of the first
binary neutron star merger detected through gravitational-wave emission, GW170817. Our …
binary neutron star merger detected through gravitational-wave emission, GW170817. Our …
Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to modeling uncertainty
… Under the Limber approximation [112,113], the 2D convergence power spectrum in
tomographic bins i and j, C ij κ (l) is related to the full 3D matter power spectrum as: …
tomographic bins i and j, C ij κ (l) is related to the full 3D matter power spectrum as: …
[PDF][PDF] Eigenvalues and eigenfunctions of ordinary differential operators
C Fefferman, L Seco - Advances in Mathematics, 1992 - core.ac.uk
… When V(x) is given by (l), our results are essentially as … Hence the successive terms uk (x)L
-’ decrease rapidly, … 9, modulo a high power of l/L With the integration constants picked in this …
-’ decrease rapidly, … 9, modulo a high power of l/L With the integration constants picked in this …