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 proposed upgrade to the LIGO detectors to form the Advanced LIGO detector system is intended to ...
Detection of gravitational waves from astrophysical sources remains one of the most challenging prob...
Detection of gravitational waves from astrophysical sources remains one of the most challenging prob...
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 ...
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 (aLIGO) detectors to enable for ...
The search for gravitational wave signals from astrophysical sources has led to the current work to ...
The search for gravitational wave signals from astrophysical sources has led to the current work to ...
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 detectors to allow the first gra...
The search for gravitational wave signals from astrophysical sources has led to the current work to ...
High purity fused silica has become the cornerstone choice for use in the final monolithic stage of ...
High purity fused silica has become the cornerstone choice for use in the final monolithic stage of ...
In 2000 the first mirror suspensions to use a quasi-monolithic final stage were installed at the GEO...
The proposed upgrade to the LIGO detectors to form the Advanced LIGO detector system is intended to ...
Detection of gravitational waves from astrophysical sources remains one of the most challenging prob...
Detection of gravitational waves from astrophysical sources remains one of the most challenging prob...
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 ...
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 (aLIGO) detectors to enable for ...
The search for gravitational wave signals from astrophysical sources has led to the current work to ...
The search for gravitational wave signals from astrophysical sources has led to the current work to ...
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 detectors to allow the first gra...
The search for gravitational wave signals from astrophysical sources has led to the current work to ...
High purity fused silica has become the cornerstone choice for use in the final monolithic stage of ...
High purity fused silica has become the cornerstone choice for use in the final monolithic stage of ...
In 2000 the first mirror suspensions to use a quasi-monolithic final stage were installed at the GEO...
The proposed upgrade to the LIGO detectors to form the Advanced LIGO detector system is intended to ...
Detection of gravitational waves from astrophysical sources remains one of the most challenging prob...
Detection of gravitational waves from astrophysical sources remains one of the most challenging prob...