Upper limit for a gravitational-wave stochastic background with the EXPLORER and NAUTILUS resonant detectors

被引：36

作者：

Astone, P

Bassan, M

Bonifazi, P

Carelli, P

Coccia, E

Cosmelli, C

Fafone, V

Frasca, S

Marini, A

Mazzitelli, G

Modena, I

Modestino, G

Moleti, A

Pallottino, GV

Papa, MA

Pizzella, G

Rapagnani, P

Ricci, F

Ronga, F

Terenzi, R

Visco, M

Votano, L

机构：

[1] IST NAZL FIS NUCL, ROME, ITALY

[2] UNIV ROMA TOR VERGATA, DIPARTIMENTO FIS, I-00173 ROME, ITALY

[3] CNR, IST FIS SPAZIO INTERPLANETARIO, I-00044 FRASCATI, ITALY

[4] UNIV AQUILA, DIPARTIMENTO FIS, I-67100 LAQUILA, ITALY

[5] IST NAZL FIS NUCL, LAQUILA, ITALY

[6] IST NAZL FIS NUCL, LAB NAZL FRASCATI, I-00044 FRASCATI, ITALY

来源：

PHYSICS LETTERS B | 1996年 / 385卷 / 1-4期

关键词：

Cosmic stochastic background; Gravitational waves; Resonant-mass gravitational wave detectors;

D O I：

10.1016/0370-2693(96)00965-3

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We discuss the sensitivity of resonant-mass gravitational-wave detectors to a cosmic stochastic background of gravitational waves. We report the experimental upper limits given by the gravitational wave detectors EXPLORER and NAUTILUS.

引用

页码：421 / 424

页数：4

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