'Gravitational wave' diaporamas de présentation

Natural Inflation after WMAP

Natural Inflation after WMAP. Katherine Freese Michigan Center for Theoretical Physics University of Michigan. TWO TYPES OF INFLATION MODELS. TUNNELING MODELS Old Inflation (Guth 1981 Chain Inflation (Freese and Spolyar 2005) tunnel through series of vacua:

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PTA and GW detection --- Lecture

PTA and GW detection --- Lecture. K. J. Lee ( ??? ) Max-Planck Institute for Radio astronomy kjlee007@gmail.com Aug. 2013. Outline. Pulsar timing array Basic physics about GW Pulsar timing response to GW Detect GW background Detect single source Practical aspects of pulsar timing array

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The Bizarre Quantum Nature of Light

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S. V. DHURANDHAR

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Bright broad-band afterglows of gravitational wave bursts from mergers of binary neutron stars

Bright broad-band afterglows of gravitational wave bursts from mergers of binary neutron stars Xuefeng Wu Purple Mountain Observatory Chinese Center for Antarctic Astronomy Chinese Academy of Sciences. Collaborators: He Gao, Xuan Ding, Bing Zhang, Zi-Gao Dai,

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VERY HIGH ENERGY PHENOMENA IN THE UNIVERSE 2014

VERY HIGH ENERGY PHENOMENA IN THE UNIVERSE 2014. A duality between the emission of micro- gravitational waves and Quantum Mechanics Vo Van Thuan Vietnam Atomic Energy Institute (VINATOM) and The Office of the State NEPIO for NPP thuanvova@gmail.com & thuanvv@moit.gov.vn

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The VIRGO experiment The commissioning of VIRGO Towards a global network Conclusions

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LIGO APS NW Section Meeting, May 30, 2003

Laser Interferometer Gravitational Wave Observatory LIGO Commissioning and Initial Science Runs: Current Status Michael Landry LIGO Hanford Observatory/Caltech on behalf of the LIGO Scientific Collaboration http://www.ligo.org. LIGO APS NW Section Meeting, May 30, 2003.

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Gravitational waves and cosmology

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Gravitational waves and cosmology

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Cosmological supernovae as neutrino and gravitational wave sources

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Gravitational Wave Observatories By: Matthew Fournier

Gravitational Wave Observatories By: Matthew Fournier. Outline. Intro to Gravitational Waves What are they Where do they come from Why are they interesting Detection Techniques Techniques Used Past, present and future detection attempts. Outline. Problems with detection Noise sources

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Hideyuki Tagoshi (Osaka Univ.) on behalf of the TAMA collaboration

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Searching for Gravitational-Wave Bursts

Searching for Gravitational-Wave Bursts. Isabel Leonor University of Oregon for the LIGO Scientific Collaboration (LSC) LIGO-G060528-01-Z. Gravitational-Wave Bursts: Sources and Searches. SNR E0102-72 NASA, Chandra, SAO, Hubble ATNF, ATCF. Astrophysical sources:.

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Gravitational Waves and LIGO

What is a Gravitational Wave? What are the sources of GW? How can we detect them? LIGO Problems with detection What can we learn from them?. Gravitational Waves and LIGO. EINSTEIN VS NEWTON. Newtonian Gravity.

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Semantics: Session 3

Semantics: Session 3. Joint Session: Semantics, VOEvent(, Theory, Registry). Agenda:. Using vocabularies VOEvent Vocabularies and the registry (SD) Discussion on how to exploit the vocabularies in a VO, e.g. by VOEvent, theory, the registry, etc.

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Study Overview

Gravitational Waves Architecting Study Workshop. Study Overview. Ken Anderson (Study Manager ). Logistics. Very tight agenda for the next two days Requires strict adherence to time limits by all parties Update to agenda: CST caucus Wednesday starting at 1:00; open discussion will follow

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Sources and Timing

LoocUp. 1 day. Wide field optical follow-up observations to gravitational wave triggers Jonah Kanner and Peter Shawhan, University of Maryland, College Park MD 20742.

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