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Several sources of noise limit the sensitivity of current gravitational wavedetectors. Currently, dominant noise sources include quantum noise and thermalBrownian noise, but future detectors will also be limited by other thermalnoise channels. In this paper we study a thermal noise source which is causedby spatial charge carrier density variations in semiconductor materials. Weprovide an analytical model for the understanding of charge carrierfluctuations under the presence of screening effects and show that chargecarrier noise will not be a limiting noise source for third generationgravitational wave detectors.

Thermal charge carrier driven noise in transmissive semiconductor optics