To further increase the sensitivity of the advanced LIGO (aLIGO) gravitational wave detectors, two major upgrades of the monolithic fused silica suspension are considered: a higher stress in the suspension fibres and a longer final suspension stage. One of the challenges for this upgrade will be producing thinner and longer fibres that can hold the test mass safely. We demonstrate that laser power fluctuations during the fibre fabrication process can produce diameter variations and potentially weak fibres. We present a laser intensity stabilisation technology for fused silica fibre fabrication using a camera system to monitor heating. Fibres fabricated with this new technique showed a 34% decrease in the interquartile range of measured brea...
The search for gravitational wave signals from astrophysical sources has led to the current work to ...
The 40 kg test masses of the Advanced LIGO interferometric gravitational wave detector will each be ...
The search for gravitational wave signals from astrophysical sources has led to the current work to ...
To further increase the sensitivity of the advanced LIGO (aLIGO) gravitational wave detectors, two m...
A pivotal aspect in increasing the sensitivity of the Advanced LIGO (aLIGO) detectors to enable for ...
The search for gravitational wave signals from astrophysical sources has led to the current work to ...
A pivotal aspect in increasing the sensitivity of the Advanced LIGO (aLIGO) detectors to enable for ...
To further increase the sensitivity of the aLIGO detectors, upgrading the monolithic fused silica su...
A pivotal aspect in increasing the sensitivity of the Advanced LIGO detectors to allow the first gra...
The observation of gravitational waves is highly influenced by the detectors sensitivity, that is li...
The 40 kg test masses of the Advanced LIGO interferometric gravitational wave detector will each be ...
The 40 kg test masses of the Advanced LIGO interferometric gravitational wave detector will each be ...
The planned upgrades to the LIGO gravitational wave detectors include monolithic mirror suspensions ...
The 40 kg test masses of the Advanced LIGO interferometric gravitational wave detector will each be ...
In 2000 the first mirror suspensions to use a quasi-monolithic final stage were installed at the GEO...
The search for gravitational wave signals from astrophysical sources has led to the current work to ...
The 40 kg test masses of the Advanced LIGO interferometric gravitational wave detector will each be ...
The search for gravitational wave signals from astrophysical sources has led to the current work to ...
To further increase the sensitivity of the advanced LIGO (aLIGO) gravitational wave detectors, two m...
A pivotal aspect in increasing the sensitivity of the Advanced LIGO (aLIGO) detectors to enable for ...
The search for gravitational wave signals from astrophysical sources has led to the current work to ...
A pivotal aspect in increasing the sensitivity of the Advanced LIGO (aLIGO) detectors to enable for ...
To further increase the sensitivity of the aLIGO detectors, upgrading the monolithic fused silica su...
A pivotal aspect in increasing the sensitivity of the Advanced LIGO detectors to allow the first gra...
The observation of gravitational waves is highly influenced by the detectors sensitivity, that is li...
The 40 kg test masses of the Advanced LIGO interferometric gravitational wave detector will each be ...
The 40 kg test masses of the Advanced LIGO interferometric gravitational wave detector will each be ...
The planned upgrades to the LIGO gravitational wave detectors include monolithic mirror suspensions ...
The 40 kg test masses of the Advanced LIGO interferometric gravitational wave detector will each be ...
In 2000 the first mirror suspensions to use a quasi-monolithic final stage were installed at the GEO...
The search for gravitational wave signals from astrophysical sources has led to the current work to ...
The 40 kg test masses of the Advanced LIGO interferometric gravitational wave detector will each be ...
The search for gravitational wave signals from astrophysical sources has led to the current work to ...