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Has elasticity anything to do with cosmology? Angelo Tartaglia RELGRAV February 17 2011 RELGRAV * “Elastic” continua xμ ξa N+n N N RELGRAV * Geometry and elasticity…
cos_kdh.ppt1 observations : H0 = 72 ± 8 km s−1 Mpc−1 t0 ≥14 ± 2 Gyr old globular clusters H0 t0 ≥1.0 ± 0.15 H0 t0 = 2 3 for ΩM
MCMC of the CMB power spectrum, and convergence Zubair and Jen Cosmology 321 ● Random samples of parameter space ● Use CAMB for numerical calculation of Cl ● Calculate…
PROBING THE INHOMOGENEOUS UNIVERSE WITH GW COSMOLOGY Kent Yagi Kyoto University (Montana State Univ. from next April) Amaldi 2011 ＠ Cardiff 7/10 2011 Atsushi Nishizawa…
KOBE BIOMEDICAL INNOVATION CLUSTER 1 Τι είναι το Kobe Biomedical Innovation Cluster KBIC Η πόλη του Kobe έχει συγκροτήσει το Kobe Biomedical…
WASH Updates February 16 , 2012 Σ= 600,000 Σ= 290,000 Σ= 970,000 Σ= 38,000 WASH Cluster KPK/FATA Update In Jalozai Camp new IDP's are arriving from Sahlobar area…
Sesi 6. Penggunaan Sampel Size dalam perhitungan. Ki Hariyadi, MPH Metode Survei Sampel UIN Sunan Kalijaga, 2015 Topik Pengantar Pengenalan Program sample size Kasus SRS…
Photometry of dwarf galaxies in the Coma clustercluster M. den Brok R. Peletier [email protected] cluster cluster cluster COMA ACS Survey: Survey will cover 740 sq. arcmin
Heavy hitters via cluster-preserving clustering Kasper Green Larsen∗ Jelani Nelson† Huy L. Nguy˜̂en‡ Mikkel Thorup§. April 5, 2016 Abstract In the turnstile `p heavy…
From quivers to derived categories and back The cluster category, and the main theorem Applications Summary Appendix: On the proof of the main theorem A characterization…
cos_kdh.ppt1 observations : H0 = 72 ± 8 km s−1 Mpc−1 t0 ≥14 ± 2 Gyr old globular clusters H0 t0 ≥1.0 ± 0.15 H0 t0 = 2 3 for ΩM
Microsoft PowerPoint - Standard Cosmology II.ppt Red shiftRed shift Hubble lawHubble law Astroparticle Course 2 The full solutions to the Friedmann equations can be quite
4 Friedmann–Robertson–Walker Universe We shall now apply the Einstein equation to the homogeneous and isotropic case, which leads to Friedmann–Robertson–Walker (FRW)…
Ψ-Epistemic Quantum Cosmology Peter W Evans∗1 Sean Gryb†2 and Karim P Y Thébault‡3 1School of Historical and Philosophical Inquiry University of Queensland 2Institute…
ASIC needs for “observational cosmology” Gary S Varner University of Hawai’i HEPIC 2013 LBNL May 30th 2013 2 What’s in out • Very broad topic minimize overlap with…
Astron. Astrophys. 342, 153–166 (1999) ASTRONOMY AND ASTROPHYSICS Seismology of δ Scuti stars in the Praesepe cluster I. Ranges of unstable modes as predicted by linear…
ASTROPHYSICS B-type pulsators in the open cluster NGC 884 (χ Persei) J. Krzesinski1 and A. Pigulski2 1 Mt. Suhora Observatory, Cracow Pedagogical University, ul. Podchorazych
S1 Supporting Information γ-Alumina-Supported Pt17 Cluster: Controlled Loading Geometrical Structure and Size-Specific Catalytic Activity for Carbon Monoxide and Propylene…
Cluster Structures on Drinfeld Doubles M. Gekhtman joint with M. Shapiro and A. Vainshtein Gone Fishing 2014 M. Gekhtman joint with M. Shapiro and A. VainshteinCluster Structures…
A member of the Central Highlands Cluster Ministry St George’s Trentham 900am St Mary’s Woodend 1100am 23rd April 2017 – Second Sunday of Easter and St George’s Day!…