Principal Investigators: H. Lück, K. Danzmann
The aim of this project is the analysis of synchronous tracking of
signals from inspiralling binary systems in continuation of the work started in Project
C1 in the last funding period. The signal from an inspiralling binary system of two
compact objects spans a wide frequenc range over the whole inspiral process but only occupies
a well predicted, narrow frequency space per unit of time for most of the event.
Instead of using a detector with a stationary tuning we investigate the response if the tuning is changed during
the inspiral event. When the tuning frequency of a signal recycled gravitational
wave detector is suddenly changed the response of the interferometer can no
longer be described by the steady state filter functions. We will develop a code for modelling the
dynamical response of a dual recycled detector and compute the
improvement of dynamical tuning in comparison to fixed-frequency
detection.
Furthermore we want to optimize the detection efficiency
and parameter estimation accuracy for GEO HF (a series of sequential
upgrades of GEO600 in the time frame 2007-2014) for
likely interferometer configurations and for scientifically
interesting sources in close cooperation with the GEO HF design
team to weigh scientifically beneficial sensitivity curves against
technical, financial and time constraints. The configurations considered include
the injection of squeezed light, changing from detuned to tuned operation and a change from
heterodyne readout to DC readout.
Former Associates | |||
| Harald Lueck | Staff, PI 2007 | ||
| Dmitry Simakov | PostDoc, 2009 |
[1]
The upgrade of GEO 600
H. Lück, C. Affeldt, J. Degallaix, A. Freise, H. Grote, M. Hewitson, S. Hild, J. Leong, M. Prijatelj, K.A. Strain, B. Willke, H. Wittel and K. Danzmann,
submitted to J. Phys. Conf. Ser.
[2]
The upgrade of GEO 600
H. Lück for the LIGO Scientific Collaboration,
MG12 conference proceedings
[3]
DC-readout of a signal-recycled gravitational wave detector
,
Class. and Quantum Grav., 26,5 , pp. 55012-55021(10), (2009)
[4]
Phenomenological template family for black-hole coalescence waveforms
P. Ajith, S. Babak, Y. Chen, M. Hewitson, B. Krishnan, J. T. Whelan, B. Bruegmann, P. Diener, J. A. Gonzalez, M. Hannam, S. Husa, M. Koppitz, D. Pollney, L. Rezzolla, L. Santamaria, A. M. Sintes, U. Sperhake, and J. Thornburg,
Class. Quantum Grav. 24, S689 (2007)
[5]
Commissioning of advanced, dual-recycled gravitational-wave detectors: simulations of complex optical systems guided by the phasor picture,
M. Malec,
PhD Thesis