London Centre for Nanotechnology, University College London, 17-19 Gordon Street, London WC1H 0AH, UK.
Institute of Structural and Molecular Biology, University College London, Gower Street, London WC1E 6BT, UK.
Sci Rep. 2017 Feb 7;7:41836. doi: 10.1038/srep41836.
The performance of a room temperature, zero-field MASER operating at 1.45 GHz has been examined. Nanosecond laser pulses, which are essentially instantaneous on the timescale of the spin dynamics, allow the visible-to-microwave conversion efficiency and temporal response of the MASER to be measured as a function of excitation energy. It is observed that the timing and amplitude of the MASER output pulse are correlated with the laser excitation energy: at higher laser energy, the microwave pulses have larger amplitude and appear after shorter delay than those recorded at lower laser energy. Seeding experiments demonstrate that the output variation may be stabilized by an external source and establish the minimum seeding power required. The dynamics of the MASER emission may be modeled by a pair of first order, non-linear differential equations, derived from the Lotka-Volterra model (Predator-Prey), where by the microwave mode of the resonator is the predator and the spin polarization in the triplet state of pentacene is the prey. Simulations allowed the Einstein coefficient of stimulated emission, the spin-lattice relaxation and the number of triplets contributing to the MASER emission to be estimated. These are essential parameters for the rational improvement of a MASER based on a spin-polarized triplet molecule.
已对在 1.45GHz 下工作的室温、零场 MASER 的性能进行了研究。纳秒激光脉冲在自旋动力学的时间尺度上基本上是瞬时的,这使得 MASER 的可见光到微波的转换效率和时间响应可以作为激发能量的函数进行测量。观察到 MASER 输出脉冲的定时和幅度与激光激发能量相关:在更高的激光能量下,微波脉冲的幅度更大,并且比在较低激光能量下记录的脉冲延迟更短。种实验证明,外部源可以稳定输出变化,并确定所需的最小种功率。MASER 发射的动力学可以通过一对一阶、非线性微分方程来建模,这些方程源自洛特卡-沃尔泰拉模型(捕食者-猎物),其中谐振器的微波模式是捕食者,而五苯三重态中的自旋极化是猎物。通过模拟,我们可以估计受激辐射的爱因斯坦系数、自旋晶格弛豫以及对 MASER 发射有贡献的三重态的数量。这些对于基于极化三重态分子的 MASER 的合理改进是必不可少的参数。