Team

Junior-Professorin Dr. rer. nat. Katharina-Sophie Isleif

Katharina is a physicist and junior professor of metrology at HSU. In her research group she investigates optical laser interferometers and sensors for measuring gravitational waves, seismic waves and dark matter such as axion-like particles. The goal is to find smart and compact interferometer solutions for various applications and make them available also for industry. For this, they are researching and developing alternative interferometer techniques, such as digital interferometry. You can find her different research projects here.

Holstenhofweg 85, 22043 Hamburg
Gebäude H02 – 2808
Tel: – 3225
Twitter: @katha_slf

Dr. Julius Grimm (Postdoc)

Julius works on numerical simulations for the future gravitational-wave detector Einstein Telescope within the BMFTR-funded project “ErUM-SESAM”. His research focuses on Newtonian noise induced by seismic waves and its impact on the detector’s sensitivity. As the geophysicist in our team, he also contributes his expertise to Distributed Acoustic Sensing (DAS) measurement campaigns and the optimisation of sensor networks for Newtonian noise mitigation.

Holstenhofweg 85, 22043 Hamburg
Gebäude H02 – 2807

Sangmin An (PhD student)

Sangmin works on a dtec.bw project “Digital Sensor-2-Cloud Campus-Plattform” and designs new optical interferometer concepts. He investigates new optical designs using IfoCAD software and then tests them in the laser lab on the HSU campus. The goal is to develop wireless, stand-alone optical sensor with high precision and at the same time high robustness (high dynamic range). For this, he uses deep frequency modulation interferometry.

Holstenhofweg 85, 22043 Hamburg
Gebäude H02 – 2807

Eleni Minakaki (PhD student)

Eleni works on portable, passive ring laser gyroscopes within the DFG Research Unit “RING”. She explores novel concepts in the laboratory and investigates the limitations of existing systems through optical simulations and modelling. Her research aims to better understand the fundamental limiting effects, develop innovative approaches, and pave the way for the next generation of high-precision ring laser gyroscopes.

Holstenhofweg 85, 22043 Hamburg
Gebäude H02 – 2807

Paul Ophardt (PhD student)

Paul works on numerical simulations for seismic waves and noise in Gravitational Wave detectors and he makes predictions for Newtonian noise in the Einstein Telescope. He optimises sensor networks and investigates filtering strategies to cancel Newtonian noise in gravitational wave detectors. His work is carried out in the framework of DASHH and will use machine learning to improve the seismic simulations.

Holstenhofweg 85, 22043 Hamburg
Gebäude H02 – 2809

Reinhardt Rading (PhD student)

Reinhardt uses and develops optical technologies to measure seismic noise, which limits high-precision experiments such as gravitational wave detectors. Among other things, he analyses DAS systems in cooperation with the WAVE team at the Bahrenfeld research campus and is also developing new readout systems for fibre sensors to increase sensitivity by using digital-assisted interferometry. This is particularly important for the planned gravitational wave detector in Europe, the Einstein Telescope. To this end, he is researching which sensor configuration and positioning can be used to suppress so-called Newtonian noise.

You can find more information about Reinhardt here.

Holstenhofweg 85, 22043 Hamburg
Gebäude H02 – 2807

Wanda Vossius (PhD student)

Wanda is working on the design of new fiber sensors to measure seismic noise with high precision at low frequencies dedicated as Newtonian Noise sensor network for the planned gravitational wave detector in Europe Einstein Telescope. She is investigating the properties of fiber Bragg gratings, mirrors, and oscillators introduced into the fiber, and how they accommodate different degrees of freedom of seismic signals. In a side project together with the University of Hamburg, Wanda has also set up a homodyne quadrature interferometer to investigate the quality and resonance frequency changes of a suspended test mass in the presence of temperature gradients. Additionally, she supports the WAVE team and especially the outreach acitivities also in social media.

Holstenhofweg 85, 22043 Hamburg
Gebäude H02 – 2807

Spiridon Beis (student assistant)

Spiridon is studying physics in Aachen. At HSU, he actively supports the WAVE team remotely as a student assistant by analysing data and monitoring the live streams on Twitch and social media. Spiridon is in the Einstein Telescope Collaboration, where he works on Newtonian Noise Cancellation and does simulations for sensor optimisation.

Aachen

Judith Nabel (team assistance)

Judith supports the metrology group with any kind of administration and organization.

Holstenhofweg 85, 22043 Hamburg
Gebäude H11