Demonstration of thermal limit mean transverse energy from cesium antimonide photocathodes

Author:

Kachwala Alimohammed1ORCID,Saha Pallavi1ORCID,Bhattacharyya Priyadarshini1ORCID,Montgomery Eric2ORCID,Chubenko Oksana3ORCID,Karkare Siddharth1ORCID

Affiliation:

1. Department of Physics, Arizona State University 1 , Tempe, Arizona 85287, USA

2. Euclid Beamlabs, LLC 2 , Beltsville, Maryland 20705, USA

3. Department of Physics, Northern Illinois University 3 , DeKalb, Illinois 60115, USA

Abstract

The mean transverse energy (MTE) of electrons emitted from cathodes is a critical parameter that determines the brightness of electron beams for applications, such as x-ray free electron lasers, particle colliders, and ultrafast electron scattering experiments. Achieving a MTE close to the thermal limit is a key step toward realizing the full potential of electron sources in these applications. Cesium antimonide (Cs3Sb) is a technologically important material with a long history of use in photon detection and electron sources. The smallest MTE of electrons photoemitted from Cs3Sb has always been appreciably greater than the thermal limit and was attributed to surface non-uniformities. In this work, we present comprehensive measurements of the photoemission electron energy spectra (PEES), quantum efficiency, and MTE from Cs3Sb in a wide photoexcitation energy range from 1.5 to 2.3 eV. Our PEES measurements demonstrate a notably low photoemission threshold of around 1.5 eV, which is in contrast with the previously perceived threshold of 1.8–2.0 eV. Moreover, we show that the MTE at this threshold of 1.5 eV nearly converges to the thermal limit at 300 K. At 1.8 eV, the MTE measured is 40 meV, which is comparable to the previously reported value. We conclude that this MTE value at 1.8 eV photon energy is not due to surface roughness effects as previously believed, but is a direct consequence of the excess energy.

Funder

National Science Foundation

U.S. Department of Energy

Publisher

AIP Publishing

Subject

Physics and Astronomy (miscellaneous)

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