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matter discoverable with future gravitational wave interferometers? Join GRAPPA as a PhD candidate within the ERC Advanced Grant “De Tenebris” (PI: G. Bertone) and develop precision models of binary black
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EU programme Is the Job related to staff position within a Research Infrastructure? No Offer Description Help us pioneer gravitational wave probes of dark matter. Do you want to work at the interface
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related to staff position within a Research Infrastructure? No Offer Description Join a pioneering PhD project exploring how massive stars evolve into gravitational-wave sources. Combine stellar physics
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between high- and low-density flows, and effect of submarine canyon dynamics such as tides, internal waves, nepheloid layers, and up- and downwelling. This body of work suggests that conventional
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, the KM3NeT neutrino telescope in the Mediterranean, the Virgo gravitational waves interferometer in Pisa, the Xenon-nT dark matter experiment in Gran Sasso, the Pierre Auger cosmic ray observatory in Argentina
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the research collaborations Nikhef participates in are the ALICE, ATLAS and LHCb experiments at CERN, the KM3NeT neutrino telescope in the Mediterranean, the Virgo gravitational waves interferometer in Pisa
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basal layers, substrate erosion, flow ignition, the distinction between high- and low-density flows, and effect of submarine canyon dynamics such as tides, internal waves, nepheloid layers, and up- and
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unique high-precision radio frequency ion trap in which single Ba+ ions will be confined and cooled to their motional ground state. With optical standing waves the individually ions will be addressed
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at the same time the available space is reduced. The project will be carried out in a team of 3 PhD researchers, one at the gravitational-wave research group at the at Nikhef and two at the department
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such as travelling waves, spirals and spots. The precise topic of your thesis can be tuned to your interests and background; see https://pub.math.leidenuniv.nl/~hupkeshj for a flavour of past research