The frequency of a 700 mW monolithic non-planar Nd:YAG ring laser (NPRO) depends with a large coupling coefficient (some MHz/mW) on the power of its laser-diode pump source. Using this effect we demonstrate the frequency stabilization of an NPRO to a frequency reference by feeding back to the current of its pump diodes.We achieved an error point frequency noise smaller than 1 mHz/ √ Hz, and simultaneously a reduction of the power noise of the NPRO by 10 dB without an additional power stabilization feed-back system. Due to the demanding requirements of recent experiments in quantum optics, laser spectroscopy and laser metrology there has been much interest in laser stabilization over the last years. Although very good stability was achieved with Ar + lasers 1 , diode-laser pumped solid-state lasers were chosen for almost all modern highprecision experiments. The reason for this choice is that the free-running frequency noise of these lasers is 2 to 3 orders of magnitude smaller than for Ar + lasers, and the intensity noise of solid-states-laser is also much lower. Furthermore, solid-state lasers have a very high electrical-to-optical efficiency, which is important especially in space applications like inter-satellite communication or high power applications as laser interferometric gravitational wave detectors.Many of these experiments rely on the high intrinsic stability of Nd:YAG non-planar ring oscillators (NPRO) 2 , the output of which is used in the experiment directly or is amplified either by injection locking [3][4][5] or in a configuration with master oscillator and power amplifier 6 . The free-running frequency noise spectral density of NPROs is of the order of 1 kHz/ √ Hz at 10 Hz and falls like 1/f at higher frequencies. The unstabilized power noise of such lasers has a level of 10 −7 / √ Hz. Although this intrinsic stability is quite high, experiments like gravitational wave detectors require a frequency stability in the mHz/ √ Hz range, and simultaneously the power noise needs to be reduced by at least an order of magnitude.The commonly used schemes to reduce the frequency noise of NPROs rely on stabilizing the laser frequency to a fixed-spacer reference cavity or an atomic resonance by feeding back to two different actuators: the temperature of the Nd:YAG crystal in the low Fourier frequency range below 1 Hz, and for higher frequencies to a piezoelectrical transducer (PZT) mounted on top of the crystal that changes the laser frequency due to stress-induced birefringence. The resonances of the PZT above 100 kHz limit the useful bandwidth of the latter actuator. Good results were achieved especially by using an additional external phase shifter (Pockels cell) as a fast actuator to increase the unity gain frequency of the feed-back control loop up to 1 MHz. For example Bondu et al.7 report a frequency noise spectral density below 10 −4 Hz/ √ Hz with respect to the reference cavity (in-loop) and in the order of 10 −2 Hz/ √ Hz with respect to an independent cavity (out-of-loop).Although these re...