Open main menu
Home
Random
Recent changes
Special pages
Community portal
Preferences
About Wikipedia
Disclaimers
Incubator escapee wiki
Search
User menu
Talk
Dark mode
Contributions
Create account
Log in
Editing
MiniGrail
(section)
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
{{Infobox telescope}} '''MiniGRAIL''' was a third-generation [[Gravitational-wave_observatory#Resonant_mass_antennas|resonant mass antenna]],<ref name="A First Course in General Relativity">{{cite book | url=https://archive.org/details/firstcourseingen00bern_0/page/214 | title=A First Course in General Relativity | publisher=Cambridge | author=Schutz , Bernard | pages=[https://archive.org/details/firstcourseingen00bern_0/page/214 214β220] | isbn=978-0521887052 | edition=2nd | date=2009-05-14 | url-access=registration }}</ref> a massive sphere designed to detect [[gravitational wave]]s. The MiniGRAIL was the first such detector to use a spherical design. It is located at [[Leiden University]] in the [[Netherlands]]. The project was managed by the [[Kamerlingh Onnes Laboratory]].<ref name="cqg20">{{cite journal | author=de Waard, A |display-authors=etal | title=MiniGRAIL, the first spherical detector | date=2003 | journal=Classical and Quantum Gravity | volume=20 | issue=10 | pages=S143βS151 | doi=10.1088/0264-9381/20/10/317 |bibcode = 2003CQGra..20S.143D |s2cid=250902916 }}</ref> A team from the Department of Theoretical Physics of the [[University of Geneva]], [[Switzerland]], was also heavily involved. The project was terminated in 2005. Gravitational waves are a type of radiation that is emitted by objects that have mass and are undergoing acceleration. The strongest sources of gravitational waves are suspected to be [[compact object]]s such as [[neutron star]]s and [[black hole]]s. This detector may be able to detect certain types of instabilities in rotating single and binary neutron stars, and the merger of small black holes or neutron stars.<ref name="Houwelingen02">{{cite web | first=Jeroen | last=Van Houwelingen | date=2002-06-24 | title=Development of a superconducting thin-film Nb-coil for use in the MiniGRAIL transducers | publisher=[[Leiden University]] | pages=1β17 | url=http://www.minigrail.nl/Student/Jeroen-report.pdf | accessdate=2009-09-16 }}</ref>
Edit summary
(Briefly describe your changes)
By publishing changes, you agree to the
Terms of Use
, and you irrevocably agree to release your contribution under the
CC BY-SA 4.0 License
and the
GFDL
. You agree that a hyperlink or URL is sufficient attribution under the Creative Commons license.
Cancel
Editing help
(opens in new window)