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Synchrotron radiation Mossbauer spectra of a rotating absorber with implications for testing velocity and acceleration time dilation

机译:旋转吸收器的同步辐射Mossbauer光谱对测试速度和加速时间的影响

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Many Mossbauer spectroscopy (MS) experiments have used a rotating absorber in order to measure the second-order transverse Doppler (TD) shift, and to test the validity of the Einstein time dilation theory. From these experiments, one may also test the clock hypothesis (CH) and the time dilation caused by acceleration. In such experiments the absorption curves must be obtained, since it cannot be assumed that there is no broadening of the curve during the rotation. For technical reasons, it is very complicated to keep the balance of a fast rotating disk if there are moving parts on it. Thus, the Mossbauer source on a transducer should be outside the disk. Friedman and Nowik have already predicted that the X-ray beam finite size dramatically affects the MS absorption line and causes its broadening. We provide here explicit formulas to evaluate this broadening for a synchrotron Mossbauer source (SMS) beam. The broadening is linearly proportional to the rotation frequency and to the SMS beam width at the rotation axis. In addition, it is shown that the TD shift and the MS line broadening are affected by an additional factor assigned as the alignment shift which is proportional to the frequency of rotation and to the distance between the X-ray beam center and the rotation axis. This new shift helps to align the disk's axis of rotation to the X-ray beam's center. To minimize the broadening, one must focus the X-ray on the axis of the rotating disk and/or to add a slit positioned at the center, to block the rays distant from the rotation axis of the disk. Our experiment, using the Fe-57 SMS, currently available at the Nuclear Resonance beamline (ID18) at the ESRF, with a rotating stainless steel foil, confirmed our predictions. With a slit installed at the rotation axis (reducing the effective beam width from 15.6 mu m to 5.4 mu m), one can measure a statistically meaningful absorption spectrum up to 300 Hz, while, without a slit, such spectra could be obtained up to 100 Hz only. Thus, both the broadening and the alignment shift are very significant and must be taken into consideration in any rotating absorber experiment. Here a method is offered to measure accurately the TD shift and to test the CH.
机译:许多Mossbauer光谱(MS)实验都使用旋转吸收器来测量二阶横向多普勒(TD)位移,并测试爱因斯坦时间膨胀理论的有效性。从这些实验中,还可以测试时钟假设(CH)和加速引起的时间膨胀。在这种实验中,必须获得吸收曲线,因为不能假定旋转过程中曲线没有展宽。由于技术原因,如果快速旋转的磁盘上有活动部件,则要保持其平衡非常复杂。因此,换能器上的Mossbauer源应位于磁盘外部。 Friedman和Nowik已经预测到X射线束的有限大小会极大地影响MS吸收线并引起其展宽。我们在这里提供明确的公式,以评估同步加速器Mossbauer源(SMS)光束的展宽。加宽与旋转频率和旋转轴上的SMS光束宽度成线性比例。另外,示出了TD偏移和MS线加宽受到分配为对准偏移的附加因素的影响,该附加因素与旋转频率以及X射线束中心与旋转轴之间的距离成比例。这种新的移位有助于使磁盘的旋转轴与X射线束的中心对齐。为了最小化展宽,必须将X射线聚焦在旋转盘的轴上和/或添加位于中心的狭缝,以阻挡远离盘旋转轴的射线。我们使用Fe-57 SMS(目前可在ESRF的核共振束线(ID18)上使用)和旋转的不锈钢箔进行的实验证实了我们的预测。通过在旋转轴上安装狭缝(将有效光束宽度从15.6μm减小到5.4μm),可以测量高达300 Hz的具有统计意义的吸收光谱,而如果没有狭缝,则可以获得直至仅100 Hz。因此,加宽和对准偏移都非常重要,并且在任何旋转吸收器实验中都必须考虑到。这里提供了一种方法,可以准确地测量TD偏移并测试CH。

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