The Big Bang Observer: High laser power for gravitational wave astrophysics

Gregory M. Harry; William Folkner; Peter Fritschel; E. Sterl Phinney; Daniel A. Shaddock

doi:10.1109/CLEO.2007.4453737

The Big Bang Observer: High laser power for gravitational wave astrophysics

Gregory M. Harry^*
, William Folkner
, Peter Fritschel
, E. Sterl Phinney
, Daniel A. Shaddock

^*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceeding › Conference Paper › peer-review

1 Citation (Scopus)

Abstract

The Big Bang Observer(BBO) is a proposed space-based gravitational wave detector which will look for the stochastic background of gravitational waves from the early universe. The positions of three free test masses, 50,000 km apart, will be monitored by laser interferometry. To reduce noise, 300 W of 355 nm light obtained from frequency-tripling the output of Nd:YAG lasers will be used. These lasers and other technology necessary for BBO will require significant research before a potential launch date of 2025.

Original language	English
Title of host publication	Conference on Lasers and Electro-Optics, 2007, CLEO 2007
DOIs	https://doi.org/10.1109/CLEO.2007.4453737
Publication status	Published - 2007
Externally published	Yes
Event	Conference on Lasers and Electro-Optics, 2007, CLEO 2007 - Baltimore, MD, United States Duration: 6 May 2007 → 11 May 2007

Publication series

Name	Conference on Lasers and Electro-Optics, 2007, CLEO 2007

Conference

Conference	Conference on Lasers and Electro-Optics, 2007, CLEO 2007
Country/Territory	United States
City	Baltimore, MD
Period	6/05/07 → 11/05/07

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10.1109/CLEO.2007.4453737

Cite this

@inproceedings{4e993d93916f4038ae91ff94eefee02e,

title = "The Big Bang Observer: High laser power for gravitational wave astrophysics",

abstract = "The Big Bang Observer(BBO) is a proposed space-based gravitational wave detector which will look for the stochastic background of gravitational waves from the early universe. The positions of three free test masses, 50,000 km apart, will be monitored by laser interferometry. To reduce noise, 300 W of 355 nm light obtained from frequency-tripling the output of Nd:YAG lasers will be used. These lasers and other technology necessary for BBO will require significant research before a potential launch date of 2025.",

author = "Harry, \{Gregory M.\} and William Folkner and Peter Fritschel and Phinney, \{E. Sterl\} and Shaddock, \{Daniel A.\}",

year = "2007",

doi = "10.1109/CLEO.2007.4453737",

language = "English",

isbn = "9781557528346",

series = "Conference on Lasers and Electro-Optics, 2007, CLEO 2007",

booktitle = "Conference on Lasers and Electro-Optics, 2007, CLEO 2007",

note = "Conference on Lasers and Electro-Optics, 2007, CLEO 2007 ; Conference date: 06-05-2007 Through 11-05-2007",

}

Harry, GM, Folkner, W, Fritschel, P, Phinney, ES & Shaddock, DA 2007, The Big Bang Observer: High laser power for gravitational wave astrophysics. in Conference on Lasers and Electro-Optics, 2007, CLEO 2007., 4453737, Conference on Lasers and Electro-Optics, 2007, CLEO 2007, Conference on Lasers and Electro-Optics, 2007, CLEO 2007, Baltimore, MD, United States, 6/05/07. https://doi.org/10.1109/CLEO.2007.4453737

TY - GEN

T1 - The Big Bang Observer

T2 - Conference on Lasers and Electro-Optics, 2007, CLEO 2007

AU - Harry, Gregory M.

AU - Folkner, William

AU - Fritschel, Peter

AU - Phinney, E. Sterl

AU - Shaddock, Daniel A.

PY - 2007

Y1 - 2007

N2 - The Big Bang Observer(BBO) is a proposed space-based gravitational wave detector which will look for the stochastic background of gravitational waves from the early universe. The positions of three free test masses, 50,000 km apart, will be monitored by laser interferometry. To reduce noise, 300 W of 355 nm light obtained from frequency-tripling the output of Nd:YAG lasers will be used. These lasers and other technology necessary for BBO will require significant research before a potential launch date of 2025.

AB - The Big Bang Observer(BBO) is a proposed space-based gravitational wave detector which will look for the stochastic background of gravitational waves from the early universe. The positions of three free test masses, 50,000 km apart, will be monitored by laser interferometry. To reduce noise, 300 W of 355 nm light obtained from frequency-tripling the output of Nd:YAG lasers will be used. These lasers and other technology necessary for BBO will require significant research before a potential launch date of 2025.

UR - https://www.scopus.com/pages/publications/82955219756

U2 - 10.1109/CLEO.2007.4453737

DO - 10.1109/CLEO.2007.4453737

M3 - Conference Paper

SN - 9781557528346

T3 - Conference on Lasers and Electro-Optics, 2007, CLEO 2007

BT - Conference on Lasers and Electro-Optics, 2007, CLEO 2007

Y2 - 6 May 2007 through 11 May 2007

ER -

The Big Bang Observer: High laser power for gravitational wave astrophysics

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