Summary
The quality factorQ of a small gravitational-wave antenna has been measured between 4.2 and 1.1 K. The dependence ofQ onT can be fitted by an expression linear in 1/T as well as by the formulaQ=Q 0 exp [Δε/kT]. In the latter case, one finds Δε≈7·10−5eV.
Riassunto
Si presentano i risultati delle misure eseguite fra 4.2 e 1.1 K del fattore di meritoQ di una piccola antenna gravitazionale. La dipendenza diQ daT può essere rappresentata da un'espressione lineare di 1/T come anche a mezzo della formulaQ=Q 0 exp [Δε/kT]. In questo secondo caso si trova Δε≈7·10−5 eV.
Резюме
В области между 4.2 и 1.1 К был измерен фактор качестваQ малой антенны гравитационных волн. ЗависимостьQ отT может быть аппроксимирована линейным выражением по 1/T, а а также формулойQ=Q 0 exp [Δε/kT]. В последнем случае находим, что Δε≈7·10−5эВ.
Similar content being viewed by others
References
J. Weber:Proc. S.I.F., Course LVI, edited byB. Bertotti (New York, N. Y., 1974), p. 263.
G. Pizzella:Estimated sensitivity of the low-temperature gravitational-wave antenna in Rome, inProceedings of the International School on Gravitational Wave, Erice, March 1975.
A. M. Fairbank, S. P. Boughn, H. J. Paik, M. S. McAshan, J. E. Opfer, R. C. Taber, W. O. Hamilton, B. Pipes, T. Bernat andJ. M. Reynolds:Proc. S.I.F., Course LVI, edited byB. Bertotti (New York, N. Y., 1974), p. 294.
a)P. Carelli, M. Cerdonio, U. Giovanardi, G. Lucano andI. Modena:Lowtemperature gravitational-radiation antenna: a progress report, inColloques Internationaux du Centre National de la Recherche Scientifique (Paris, 1973);b)E. Amaldi andG. Pizzella:The gravitational-wave experiment in Rome: Progress report, Internal Report No. 645, Istituto di Fisica dell'Università, Roma (1975);c)E. Amaldi, S. Barbanera, F. Bordoni, P. Bonifazi, M. Cerdonio, C. Cosmelli, U. Giovanardi, I. Modena, G. V. Pallottino, G. Pizzella, F. F. Ricci, G. L. Romani andG. Vannaroni:The gravitational-wave experiment in Rome: Progress report, inProceedings of the International Symposium on Experimental Gravitation, Pavia, September 1976.
W. Davis, D. Gretz, J. P. Richard, G. Rydbeck andJ. Weber:Lett. Nuovo Cimento,16, 199 (1976).
V. Braginskii:The detection of gravitational waves and quantum nondisturbative measurements, inProceedings of the International School on Gravitational Wave, Erice, March 1975.
G. Papini:V Cambridge Conference on Experimental Relativity (Cambridge, Mass., 1974).
D. Douglass:Gravitational-wave experiments, inProceedings of the International Symposium on Experimental Gravitation, Pavia, September 1976.
P. Carelli, A. Foco, U. Giovanardi, I. Modena, D. Bramanti andG. Pizzella:Q measurements down to liquid-helium temperatures for a gravitational-wave aluminium bar antenna, inCryogenics (July 1975), p. 406.
G. V. Pallottino andG. Pizzella:On the electrical equivalent circuits of multiple sensor gravitational-wave antennas, Internal Report LPS-77-9, Frascati (March 1977).
Author information
Authors and Affiliations
Additional information
Переведено редакцией.
Rights and permissions
About this article
Cite this article
Amaldi, E., Cosmelli, C., Giovanardi, U. et al. Measurements of the merit factorQ of an aluminium gravitational-wave antenna between 4.2 and 1.1 K. Nuov Cim B 41, 327–333 (1977). https://doi.org/10.1007/BF02740887
Received:
Published:
Issue Date:
DOI: https://doi.org/10.1007/BF02740887