PPT-Perturbations

Author : tatyana-admore | Published Date : 2016-06-16

Applying Perturbations in Tellurium 2 import tellurium as te import numpy r teloada Model Definition v1 Xo gt S1 k1Xo v2 S1 gt w k2S1

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Perturbations: Transcript


Applying Perturbations in Tellurium 2 import tellurium as te import numpy r teloada Model Definition v1 Xo gt S1 k1Xo v2 S1 gt w k2S1 . 3106 11 lecture9 NonlinearControlTheory2006 brPage 2br TodayTwoTimescales Averaging The state moves slowly compared to Singularperturbations 57480 The state moves slowly compared to lecture9 NonlinearControlTheory2006 brPage 3br ExampleVibratingPend The conclusion is that if we smooth the distribution on the largest scales lar ger than several hundred Mpc scales it approaches a homogeneous distribution in accord with th e assumptions that underlie the FRW model However as we go to smaller scale Frowning Smiling and Winking brPage 7br Rainbow Holograms Use 2 nd gen setup HeNe Laser Shutter Variable Beam Splitter Folding Mirrors Unexposed Film Master Hologram Variable Beam Splitter Curved Mirror Replace w cylindrical lens Reference Beam Refe 郭宗寛 . (. Zong-Kuan. . Guo. ). ITP. , . CAS. 3rd . Joint Retreat on Cosmology and LHC . Physics. November 2, 2012. Based on . collaboration . with . D.J. . . Schwarz. Phys. . Rev. D 80 (2009) 063523 [arXiv:0907.0427. http://leandros.physics.uoi.gr. Department of Physics. University of . Ioannina. Open page. Accelerating Universe:. Geometric Observational Constraints. and. Growth of Perturbations. Main Points. Recent Geometric Probe Data (SnIa, CMB, BAO). Eccentric and Mean anomalies. Kepler’s. equation. f,g. functions . Universal variables for hyperbolic and eccentric orbits. Disturbing function. Low eccentricity expansions for Disturbing function. run inefficiency. Detector issues:. increasing event size (PMD): run in a separate partition. HV, LV, … instabilities (MCH. ). Faulty HV . crate+modules. being replaced. DCS error (?). perturbations (power glitches, etc), network issues (DAQ, HLT). Priority. Project. COSMO WG7. Chiara Marsigli. COTEKINO . Priority. Project. Duration. : 2 . years. , 2013-2015. FTEs. : 5 (3 . FTEs. 2013/2014 and 2 FTE 2014/2015). Aim. : . develop. and test . perturbation. Gaussianity. from early Universe. Kazuya Koyama. University of Portsmouth. Proved by CMB anisotropies. nearly scale invariant. nearly adiabatic . nearly Gaussian. Generation mechanisms. ICRR, U Tokyo. Weak lensing of CMB. from. . cosmic (super-)strings. 9/28/2011 JGRG21 @ Tohoku U. w. ith A. . Taruya. (U Tokyo, RESCEU), T. . Namikawa. (U Tokyo), . K. Takahashi (Kumamoto U), Y. . and Large-Scale Structure. 1. Cora Dvorkin. IAS (Princeton) Harvard (Hubble fellow) . COSMO 2014. August 2014, Chicago. Outline. Dark Matter overview.. Effect of . WIMP Dark Matter . Hayato. . Motohashi. & . Teruaki. . Suyama. . (. Research Center for the Early Universe, The University of Tokyo). 1107.3705 (to appear in PRD). Alternative theories of gravity. In the weak gravitational field regime, GR is fully consistent with observations and experiments so far.. The Cosmic Bounce. Valerio . Bozza. University of Salerno, Italy. Summary. The Inflation and The String. The String and The Bounce. The Bounce and The Perturbations. The Bounce and The Inflation. Standard Inflation. Partie . 1. :. Azote – . Phosphore . Collège Lionel-Groulx. 1. Plan du cours. Cycles biogéochimiques: généralités. Le cycle de l’azote et les zones mortes océaniques. Le cycle du phosphore et l’eutrophisation.

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