Reduction of effective terahertz focal spot size by means of nested concentric parabolic reflectors

An ongoing limitation of terahertz spectroscopy is that the technique is generally limited to the study of relatively large samples of order 4 mm across due to the generally large size of the focal beam spot. We present a nested concentric parabolic reflector design which can reduce the terahertz fo...

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Main Authors: V. A. Neumann, N. J. Laurita, LiDong Pan, N. P. Armitage
Format: Article
Language:English
Published: AIP Publishing LLC 2015-09-01
Series:AIP Advances
Online Access:http://dx.doi.org/10.1063/1.4931815
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author V. A. Neumann
N. J. Laurita
LiDong Pan
N. P. Armitage
author_facet V. A. Neumann
N. J. Laurita
LiDong Pan
N. P. Armitage
author_sort V. A. Neumann
collection DOAJ
description An ongoing limitation of terahertz spectroscopy is that the technique is generally limited to the study of relatively large samples of order 4 mm across due to the generally large size of the focal beam spot. We present a nested concentric parabolic reflector design which can reduce the terahertz focal spot size. This parabolic reflector design takes advantage of the feature that reflected rays experience a relative time delay which is the same for all paths. The increase in effective optical path for reflected light is equivalent to the aperture diameter itself. We have shown that the light throughput of an aperture of 2 mm can be increased by a factor 15 as compared to a regular aperture of the same size at low frequencies. This technique can potentially be used to reduce the focal spot size in terahertz spectroscopy and enable the study of smaller samples.
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spelling doaj.art-b403856fcfa34642be9098321b313cc22022-12-22T00:02:24ZengAIP Publishing LLCAIP Advances2158-32262015-09-0159097203097203-710.1063/1.4931815066509ADVReduction of effective terahertz focal spot size by means of nested concentric parabolic reflectorsV. A. Neumann0N. J. Laurita1LiDong Pan2N. P. Armitage3Department of Physics and Astronomy, The Johns Hopkins University, Baltimore, Maryland, 21218, USADepartment of Physics and Astronomy, The Johns Hopkins University, Baltimore, Maryland, 21218, USADepartment of Physics and Astronomy, The Johns Hopkins University, Baltimore, Maryland, 21218, USADepartment of Physics and Astronomy, The Johns Hopkins University, Baltimore, Maryland, 21218, USAAn ongoing limitation of terahertz spectroscopy is that the technique is generally limited to the study of relatively large samples of order 4 mm across due to the generally large size of the focal beam spot. We present a nested concentric parabolic reflector design which can reduce the terahertz focal spot size. This parabolic reflector design takes advantage of the feature that reflected rays experience a relative time delay which is the same for all paths. The increase in effective optical path for reflected light is equivalent to the aperture diameter itself. We have shown that the light throughput of an aperture of 2 mm can be increased by a factor 15 as compared to a regular aperture of the same size at low frequencies. This technique can potentially be used to reduce the focal spot size in terahertz spectroscopy and enable the study of smaller samples.http://dx.doi.org/10.1063/1.4931815
spellingShingle V. A. Neumann
N. J. Laurita
LiDong Pan
N. P. Armitage
Reduction of effective terahertz focal spot size by means of nested concentric parabolic reflectors
AIP Advances
title Reduction of effective terahertz focal spot size by means of nested concentric parabolic reflectors
title_full Reduction of effective terahertz focal spot size by means of nested concentric parabolic reflectors
title_fullStr Reduction of effective terahertz focal spot size by means of nested concentric parabolic reflectors
title_full_unstemmed Reduction of effective terahertz focal spot size by means of nested concentric parabolic reflectors
title_short Reduction of effective terahertz focal spot size by means of nested concentric parabolic reflectors
title_sort reduction of effective terahertz focal spot size by means of nested concentric parabolic reflectors
url http://dx.doi.org/10.1063/1.4931815
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