Issues

 / 

1994

 / 

December

  

Conferences and symposia


A fourth-generation cryogenic gravitational antenna


Leiden University, Leiden, The Netherlands

Large metallic cylinders with a mass of several tons have been cooled to liquid helium temperatures and recently down to T ~ 100 mK leading to the most sensitive gravitational wave detector (NAUTILUS). The sensitivity is still not enough to detect waves from distances so large that the number of events becomes several per year. Cooling spherical detectors with a mass around 100 tons to temperatures around 10 mK could achieve this goal giving rise to a new astronomy.

PACS: 01.10.Fv, 04.80.Nn, 95.55.Ym (all)
DOI: 10.1070/PU1994v037n12ABEH000061
URL: https://ufn.ru/en/articles/1994/12/k/
Citation: Frossati G "A fourth-generation cryogenic gravitational antenna" Phys. Usp. 37 1192–1197 (1994)
BibTexBibNote ® (generic)BibNote ® (RIS) MedlineRefWorks
PT Journal Article
TI A fourth-generation cryogenic gravitational antenna
AU Frossati G
FAU Frossati G
DP 10 Dec, 1994
TA Phys. Usp.
VI 37
IP 12
PG 1192-1197
RX 10.1070/PU1994v037n12ABEH000061
URL https://ufn.ru/en/articles/1994/12/k/
SO Phys. Usp. 1994 Dec 10;37(12):1192-1197

Оригинал: Фроссати Дж «Криогенная гравитационная антенна четвертого поколения» УФН 164 1283–1288 (1994); DOI: 10.3367/UFNr.0164.199412k.1283

© 1918–2021 Uspekhi Fizicheskikh Nauk
Email: ufn@ufn.ru Editorial office contacts About the journal Terms and conditions