2006
DOI: 10.1016/j.nima.2006.06.009
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InSb cryogenic radiation detectors

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Cited by 15 publications
(9 citation statements)
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“…Moreover, some studies have shown that the s orbital of the lone‐pair electrons can cause a strong s‐p antibonding characteristic at the top of the VB, resulting in an increase of the VB dispersion and a decrease of the effective mass of electrons and holes, [ 8 ] which facilitates the migration of charge carriers. Several valuable X‐ray detection materials all contain different kinds of lone‐pair electron cations, including InSb, [ 9 ] PbI 2 , [ 10 ] BiI 3 , [ 11 ] CZT [ 5a ] and metal halide perovskites CsPbBr 3 [ 12 ] and CH 3 NH 3 SnI 3 . [ 13 ]…”
Section: Introductionmentioning
confidence: 99%
“…Moreover, some studies have shown that the s orbital of the lone‐pair electrons can cause a strong s‐p antibonding characteristic at the top of the VB, resulting in an increase of the VB dispersion and a decrease of the effective mass of electrons and holes, [ 8 ] which facilitates the migration of charge carriers. Several valuable X‐ray detection materials all contain different kinds of lone‐pair electron cations, including InSb, [ 9 ] PbI 2 , [ 10 ] BiI 3 , [ 11 ] CZT [ 5a ] and metal halide perovskites CsPbBr 3 [ 12 ] and CH 3 NH 3 SnI 3 . [ 13 ]…”
Section: Introductionmentioning
confidence: 99%
“…InSb Schottky diodes fabricated from epitaxially grown crystals had been studied as radiation detectors [9][10][11]. Cooling the Schottky diode to 42 K, alpha particles (5.5 MeV in energy) were detected with 1.8 % FWHM [11].…”
Section: Introductionmentioning
confidence: 99%
“…These diodes were cooled to very low cryogenic temperature (4.2-5.4 K) to avoid high leakage currents contributing to noise in the detection system. Using InSb wafer grown by liquid phase epitaxy, a FWHM of 2.4 % was achieved for 5.5 MeV alpha particles when the diode was cooled to 5.4 K [3].…”
Section: Introductionmentioning
confidence: 99%