Nearly collimated atomic beam is of interest for a variety of experiments. This article reports a simple way of modifying the atomic beam distribution using a dark wall oven and describes detailed study of outcoming atoms’ spatial distribution. A simple design is obtained by employing the fact that inhomogeneous thermal distribution along a capillary results due to its partial resistive heating. Based on this phenomenon, we have designed a dark wall oven consisting of a reservoir, collimator, and cold absorber at the exit end of atoms, where all three are fabricated out of a single stainless steel capillary. The nearly collimated spatial distribution of the atoms resulting due to the absorber eliminating the atoms diverging above a certain angle is modeled and experimentally verified. A divergence as minimum as 1.2(1)° corresponding to a half angle θ1/2 = 0.9(1)° is measured at an oven temperature of 250 °C that produces an atomic flux of about 8 × 109 atoms s−1. Total flux as estimated using our measured spatial distribution of atoms matches well with the numerically simulated values of it for the dark wall oven.
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Research Article|
May 10 2019
Atomic flux distribution from a low-divergent dark wall oven
Lakhi Sharma
;
Lakhi Sharma
1
CSIR–National Physical Laboratory
, Dr. K. S. Krishnan Marg, New Delhi 110012, India
2
Academy of Scientific and Innovative Research (AcSIR)
, Ghaziabad 201002, India
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A. Roy
;
A. Roy
1
CSIR–National Physical Laboratory
, Dr. K. S. Krishnan Marg, New Delhi 110012, India
2
Academy of Scientific and Innovative Research (AcSIR)
, Ghaziabad 201002, India
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S. Panja
;
S. Panja
1
CSIR–National Physical Laboratory
, Dr. K. S. Krishnan Marg, New Delhi 110012, India
2
Academy of Scientific and Innovative Research (AcSIR)
, Ghaziabad 201002, India
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a)
Electronic mail: subhadeep@nplindia.org.
Rev. Sci. Instrum. 90, 053202 (2019)
Article history
Received:
January 25 2019
Accepted:
April 20 2019
Citation
Lakhi Sharma, A. Roy, S. Panja, S. De; Atomic flux distribution from a low-divergent dark wall oven. Rev. Sci. Instrum. 1 May 2019; 90 (5): 053202. https://doi.org/10.1063/1.5090199
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