Precise Study of the Gap Response in LISA Quadrant Photodiodes
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Master Thesis
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Abstract
This thesis presents the first configuration and validation of a free-space laser
optical setup specifically designed to probe the inter-quadrant gap region of the
Quadrant Photodiodes (QPDs) developed at Nikhef and SRON for the Laser
Interferometer Space Antenna (LISA). Beam propagation through multiple
lenses was numerically simulated using the ABCD law for Gaussian beams to
characterize telescoping and collimating lens systems for coupling the beam into
an objective lens, with the latter ultimately providing the best performance. A
knife-edge (KE) technique was then employed to determine the z-positioning
of the objective lens in order to achieve the smallest possible beam spot on
the QPD. In parallel, a fully Python based data acquisition and analysis
pipeline was implemented, enabling automated KE and rasterized linescan
measurements for both "+" and "x" QPD orientations. Using this system, the
gap response to a direct current (DC) laser was investigated for three Run1
and one Run2 QPDs. For the Run1 AS_011_CC, which features the baseline
active area and gap size envisaged for LISA, a significant positive gap sensitivity
of +9.70% was measured, confirming and exceeding earlier estimates from
fiber-coupled laser uniformity measurements. Two additional Run1 devices
exhibit smaller but still positive responses (∼+1%), indicating that the gap in
QPDs from this batch contributes additional photocurrent rather than acting
as an electrically inactive region. In contrast, the Run2 B17R11, which also has
baseline dimensions, shows a negative gap sensitivity of−5.36%. This value
is close to the−7% response loss currently assumed in the LISA performance
model, but represents a worse performance from the photodiode: overall less
power is being detected. These results demonstrate that the gap region of the
LISA QPDs contributes measurably to the photocurrent in a batch dependent
manner. The optical setup and analysis framework developed in this thesis
provide the first repeatable method for quantifying the gap sensitivity and
establish the foundation for future optimization of LISA QPDs.
Keywords
LISA; gravitational waves; Quadrant Photodiode (QPD); Quadrant Photo-Receiver (QPR); interferometer; metrology; laser; Gaussian beams; heterodyne detection; semiconductor; photodiode; telescoping lens system; collimating lens system; knife-edge; responsivity; photocurrent; gap; space; binary systems; mergers;