English
 
User Manual Privacy Policy Disclaimer Contact us
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT
 
 
DownloadE-Mail
  Laser development for LISA

Tröbs, M., Weßels, P., Fallnich, C., Bode, M., Freitag, I., Skorupka, S., et al. (2006). Laser development for LISA. Classical and Quantum Gravity, 23(8), S151-S158.

Item is

Basic

show hide
Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-4C00-B Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-4C01-9
Genre: Conference Paper

Files

show Files
hide Files
:
cqg6_8_s20.pdf (Publisher version), 234KB
Name:
cqg6_8_s20.pdf
Description:
-
Visibility:
Public
MIME-Type / Checksum:
application/pdf / [MD5]
Technical Metadata:
Copyright Date:
-
Copyright Info:
eDoc_access: PUBLIC
License:
-

Locators

show

Creators

show
hide
 Creators:
Tröbs, Michael1, Author              
Weßels, P., Author
Fallnich, Carsten, Author
Bode, M., Author
Freitag, Ingo, Author
Skorupka, Sascha1, 2, Author
Heinzel, Gerhard1, Author              
Danzmann, Karsten1, Author              
Affiliations:
1Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, ou_24010              
2AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, ou_24009              

Content

show
hide
Free keywords: -
 Abstract: The two most promising configurations for the LISA laser are a stand-alone diode-pumped nonplanar ring oscillator (NPRO) or a fibre amplifier seeded by a low-power NPRO. The stand-alone laser was stabilized in frequency to a ULE cavity and in power to an electronic reference. For the first time the LISA requirement of relative power noise below 2 × 10-4/Hz1/2 was fulfilled in the whole frequency range from 0.1 mHz to 1 Hz. The LISA goal of frequency noise below 30 Hz/Hz1/2 was achieved for frequencies above 3 mHz. As a first step in the characterization of an oscillator-amplifier system, the excess frequency noise of an ytterbium-doped fibre amplifier was measured. For frequencies between 0.1 mHz and 1 Hz the excess noise was measured to be below 0.1 Hz/Hz1/2, which is significantly below the free-running frequency noise of NPROs.

Details

show
hide
Language(s):
 Dates: 2006
 Publication Status: Published in print
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Method: -
 Identifiers: eDoc: 265181
DOI: 10.1088/0264-9381/23/8/S20
 Degree: -

Event

show
hide
Title: 6th Edoardo Amaldi Conference On Gravitational Waves
Place of Event: Okinawa, Japan
Start-/End Date: 2005-06-20 - 2005-06-24

Legal Case

show

Project information

show

Source 1

show
hide
Title: Classical and Quantum Gravity
Source Genre: Journal
 Creator(s):
Affiliations:
Publ. Info: -
Pages: - Volume / Issue: 23 (8) Sequence Number: - Start / End Page: S151 - S158 Identifier: ISSN: 0264-9381