Differences between revisions 2 and 10 (spanning 8 versions)
Revision 2 as of 2010-04-12 21:16:08
Size: 530
Editor: AidanBrooks
Comment:
Revision 10 as of 2010-04-12 21:30:54
Size: 611
Editor: AidanBrooks
Comment:
Deletions are marked like this. Additions are marked like this.
Line 1: Line 1:
|||||||<style="text-align: center;"> '''''future meetings''''' ||
|| '''date''' || '''lead''' || '''article''' || '''lead comment''' ||
|| Apr 08, 2010 || Alastair Heptonstall ||[http://prd.aps.org/abstract/PRD/v79/i12/e122002] ||''Prospects of higher-order Laguerre-Gauss modes in future gravitational wave detectors'' ||
|| Apr 15, 2010 || Alex Mott || || ||
|| Apr 22, 2010 || Zach Korth || || ||
|| Apr 29, 2010 || Frank Seifert || || ||
|| May 06, 2010 || Izumi Kiwamu || || ||
|| May 13, 2010 || Greg Ogin || || ||
|| '''Done?''' || '''article''' || '''lead comment''' ||
|| '''done''' || [http://prd.aps.org/abstract/PRD/v79/i12/e122002] ||''Prospects of higher-order Laguerre-Gauss modes in future gravitational wave detectors'' ||
|| || Physics '''3''', 32 (2010) [http://physics.aps.org/viewpoint-for/10.1103/PhysRevLett.104.153901] || ''Second-harmonic generation in microresonators through natural phase matching'' ||
|| || Physics '''3''', 29 (2010) [http://physics.aps.org/articles/v3/29] || ''Precise simulations for future gravitational wave detectors
''||
|| || || ||
|| || || ||
|| || || ||

Done?

article

lead comment

done

[http://prd.aps.org/abstract/PRD/v79/i12/e122002]

Prospects of higher-order Laguerre-Gauss modes in future gravitational wave detectors

Physics 3, 32 (2010) [http://physics.aps.org/viewpoint-for/10.1103/PhysRevLett.104.153901]

Second-harmonic generation in microresonators through natural phase matching

|| || Physics 3, 29 (2010) [http://physics.aps.org/articles/v3/29] || Precise simulations for future gravitational wave detectors ||

Journal_Club/Interesting_papers (last edited 2024-11-15 19:38:29 by AaronjonesATligoDOTorg)