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Omni-directional interferometric inertial sensor

Project description

Advanced inertial sensors for gravitational-wave astrophysics

Coupling compact interferometric sensors with a reference mass that senses signals in all directions (omnidirectional mass) will lead to revolutionary improvements in sensor sensitivity. Within the framework of the EU-funded OmniSens project, Netherland’s Stichting VU has developed a novel inertial system that will reduce residual accelerations in horizontal directions by at least two orders of magnitude at low-frequency gravitational waves (0.1 Hz). When used as the first stage of isolation in gravitational-wave detectors, the system will enable the detectors to reach their design sensitivities and will pave the way for the use of lower frequencies in observatories.

Objective

OmniSens is a novel inertial isolation system that will approach the fundamental limits imposed by materials and terrestrial gravity. Revolutionary improvements in sensitivity will come from coupling compact interferometric sensors that are beyond the state-of-the-art with a reference mass that is Omni-directionally Sensed (OmniSens). The key concept is the use of a single, geometrically-large reference mass that is sensed and softly-suspended in all six degrees of freedom, and housed within a platform that is actively controlled to be a constant distance from it. The inertial stability of the reference mass is thus transferred to the platform in a fashion mimicking the drag-free control of a satellite around a free-floating proof mass.

Compared with the state-of-the-art, OmniSens will reduce residual accelerations in horizontal directions by at least 2 orders of magnitude at 0.1Hz. When this system is used as the first stage of isolation in a gravitational-wave detector, it will enable current detectors to finally reach their design sensitivities and push the seismic wall to lower frequencies in future observatories.

Pushing the low frequency boundary will have two critical effects: it will increase the signal-to-noise of individual sources, thus expanding the astrophysical reach of observatories, and it will vastly augment the amount of time each source is in-band, possibly allowing sky localisation before the merger of neutron stars, with spectacular consequences for electromagnetic follow up campaigns.

To achieve these ambitious goals we will need to: Develop the test and measurement infrastructure capable of housing and measuring the reference mass; Test a prototype isolation system, showing that it can reach fundamental limits imposed by simple, metal-wire suspensions; and Build a robust OmniSens system suspended with fused-silica fibres that will become a foundational element of future gravitational-wave observatories.

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Programme(s)

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Topic(s)

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Funding Scheme

Funding scheme (or “Type of Action”) inside a programme with common features. It specifies: the scope of what is funded; the reimbursement rate; specific evaluation criteria to qualify for funding; and the use of simplified forms of costs like lump sums.

ERC-COG - Consolidator Grant

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Call for proposal

Procedure for inviting applicants to submit project proposals, with the aim of receiving EU funding.

(opens in new window) ERC-2019-COG

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Host institution

STICHTING VU
Net EU contribution

Net EU financial contribution. The sum of money that the participant receives, deducted by the EU contribution to its linked third party. It considers the distribution of the EU financial contribution between direct beneficiaries of the project and other types of participants, like third-party participants.

€ 1 606 331,00
Address
DE BOELELAAN 1105
1081 HV Amsterdam
Netherlands

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Activity type
Higher or Secondary Education Establishments
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Total cost

The total costs incurred by this organisation to participate in the project, including direct and indirect costs. This amount is a subset of the overall project budget.

€ 1 606 331,00

Beneficiaries (2)

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