auriga.lnl.infn.it

AURIGA Home Page

Welcome to the AURIGA detector. The AURIGA project aims at detecting gravitational waves impinging on the Earth from the Universe. The detector is based on a very low losses ultracryogenic mechanical oscillator: when a burst of gravitational waves hits and excites the oscillator, this will vibrate for a time span much longer than the duration of the burst (typically 1msec), thus allowing the extraction of the signal from the detector noise. Learn more on gravitational waves. AURIGA is a INFN.

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AURIGA Home Page | auriga.lnl.infn.it Reviews

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Welcome to the AURIGA detector. The AURIGA project aims at detecting gravitational waves impinging on the Earth from the Universe. The detector is based on a very low losses ultracryogenic mechanical oscillator: when a burst of gravitational waves hits and excites the oscillator, this will vibrate for a time span much longer than the duration of the burst (typically 1msec), thus allowing the extraction of the signal from the detector noise. Learn more on gravitational waves. AURIGA is a INFN.

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1 experiment at lnl

2 bulletin board

3 internal

4 internal use only

5 old bulletin board

6 visit our forum

7 auriga online monitor

8 latest news

9 past auriga news

10 scientific results

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AURIGA Home Page | auriga.lnl.infn.it Reviews

https://auriga.lnl.infn.it

Welcome to the AURIGA detector. The AURIGA project aims at detecting gravitational waves impinging on the Earth from the Universe. The detector is based on a very low losses ultracryogenic mechanical oscillator: when a burst of gravitational waves hits and excites the oscillator, this will vibrate for a time span much longer than the duration of the burst (typically 1msec), thus allowing the extraction of the signal from the detector noise. Learn more on gravitational waves. AURIGA is a INFN.

INTERNAL PAGES

auriga.lnl.infn.it

1

Brief on gravitational waves

http://www.auriga.lnl.infn.it/auriga/grav_wave.html

Gw) are predicted by General Relativity. They are generated by accelerated motion of bodies, which must have quadrupolar or higher order symmetry. Detectable signals are expected only by massive, compact celestial bodies as for instance two neutron stars or black holes in orbit in a binary system or vibration of black holes and neutron stars. For a description of gravitational wave sources of interest for AURIGA please follow this link. In 1993 for this research. Of interest for AURIGA .

2

AURIGA: the test facility

http://www.auriga.lnl.infn.it/auriga/test_fac/test_facility.html

The Transducer Test Facility. In order to improve the sensitivity. Of the detector, the AURIGA collaboration is working on some R&D projects. Focused on the redesign of the transducer. Chain Obviously, before implementing the new devices on the detector they must be tested in an experimental setup that mimics the final one: the detector itself cannot be used as a transducer-amplifier bench test. To this end the AURIGA collaboration developed the Transducer Test Facility ( TTF. Have an experimental chambe...

3

AURIGA: temporary positions

http://www.auriga.lnl.infn.it/auriga/temporary.html

Temporary positions at AURIGA. In AURIGA the following scholarships and fellowships are available:. Short term grants for working in the AURIGA Trento group (SQUID, capacitive transducer) are also available. Fellowships are available for the following research projects:. 16 Studio dell'effetto di disturbi locali sul rivelatore di onde gravitazionali AURIGA e sviluppo di tecniche per la loro reiezione. 19 Caratterizzazione criogenica di un trasduttore risonante ottico ottimizzato per il rivelatore AURIGA.

4

AURIGA: the SQUID R&D project

http://www.auriga.lnl.infn.it/auriga/RandD/squid.html

AURIGA: R&D project on the SQUID. The SQUID behavior is explained by a theory which is well confirmed by the experimental data. According to this theory, the power spectral density of the voltage noise at the SQUID output is:. Represents value of the shunt resistances included in the SQUID sensor. As this noise is linearly proportional to the SQUID working temperature and vanishes at the absolute zero, we can call it thermal noise. For a typical thin film SQUID we have R. It makes negligible the noise co...

5

AURIGA: useful links

http://www.auriga.lnl.infn.it/auriga/links.html

A list of useful links. Gravitational wave detector community:. Resonant bar detectors: ALLEGRO. Resonant spherical detectors: MiniGRAIL. Wideband acoustic detector: DUAL. The resonant detectors international network: IGEC. The Gravitational Wave International Committee: GWIC. Http:/ www.batse.msfc.nasa.gov/. NASA site on GRB. Http:/ www.phys.lsu.edu/mog/. Http:/ vizier.u-strasbg.fr/. Library of published astronomical catalogues and data tables. Http:/ relativity.livingreviews.org/.

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gwic.ligo.org

GWIC - The Gravitational Wave International Committee

https://gwic.ligo.org/members

Member Projects and Representatives. Sheila Rowan, University of Glasgow, (GWIC, 2009- , Chair 2015- ). Bram Slagmolen, Australian National University, 2015-. Massimo Cerdonio, University of Padua and. Michele Punturo, INFN-Perugia, 2009-. European Pulsar Timing Array (EPTA). Michael Kramer, Max-Planck-Institut für Radioastronomie and Jodrell Bank Centre for Astrophysics (University of Manchester), 2009-. Karsten Danzmann, Albert-Einstein-Institut fur Gravitationsphysik and University of Hannover, 1997-.

auriga9.lnl.infn.it

AURIGA Current Status

http://auriga9.lnl.infn.it/AURIGA_STATUS/index.php

Status @ Sat 20/08/2016 09:30:46 UTC. AURIGA Channel status at Saturday 2016/08/20 - 09:30:46 UTC.

dalcanton.it

Tito Dal Canton

http://www.dalcanton.it/tito

Physics is reverse engineering. I'm an Italian guy with a passion for science and technology. Here I want to share some of the things I've done, especially related to my interests, experiments, studies and jobs. It's pretty much a bunch of hyper-technical stuff, but I hope you'll find something interesting. I studied physics in Padova and I had the pleasure of working with the AURIGA group. I'm currently a postdoc at the AEI Hannover. I work on gravitational wave. In data from the LIGO detectors.

rarenoise.lnl.infn.it

Rarenoise - background

http://www.rarenoise.lnl.infn.it/sciback.html

A project funded by the. The RareNoise project bridges two separated field of science. They are:. The research on Non Equilibrium Fluctuations. The research on Gravitational Waves. Intense gravitational radiation is predicted to be emitted by violent events occurring in the cosmos; direct detection of gravitational radiation of astrophysical origin is a very challenging task that engages scientists all over the world. Relativity and Gravitational Radiation. Living reviews in relativity. Prof D J Evans.

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AURIGA Home Page

Welcome to the AURIGA detector. The AURIGA project aims at detecting gravitational waves impinging on the Earth from the Universe. The detector is based on a very low losses ultracryogenic mechanical oscillator: when a burst of gravitational waves hits and excites the oscillator, this will vibrate for a time span much longer than the duration of the burst (typically 1msec), thus allowing the extraction of the signal from the detector noise. Learn more on gravitational waves. AURIGA is a INFN.

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