Skip to main content
U.S. flag

An official website of the United States government

Official websites use .gov
A .gov website belongs to an official government organization in the United States.

Secure .gov websites use HTTPS
A lock ( ) or https:// means you’ve safely connected to the .gov website. Share sensitive information only on official, secure websites.

Mark Tyra (Fed)

Mark Tyra is a physical scientist (isotope geochemist) in the NIST Radioactivity Group in the Radiation Physics division. For his PhD (Univ. of New Mexico) and MSc (Univ. of Maryland, College Park) work, he used radionuclide and stable isotope signatures with petrography to trace the history of water in asteroids (using meteorites). He joined the Radioactivity Group in 2013. 

Currently, Mark is the primary contact in a project that will expand the capability of NIST’s to calibrate short-lived radioisotopes using a secondary ionization chamber. He also uses mass spectrometry to analyze radioactive and stable isotope composition of materials to be used as reference materials for the medical isotope, nuclear, and other applications. He participates in a collaborations for improving calibrations of ionizing radionuclide solutions, detection of impurities in medical radiopharmaceuticals, nuclear forensics measurements, neutrino detection, neutron lifetime, and others.

Projects and Collaborations

Opportunities

Professional Affiliations and Service

Publications

Limits on Strongly Interacting Sub-GeV Dark Matter from the PROSPECT Reactor Antineutrino Experiment

Author(s)
Hans Pieter Mumm, Denis E. Bergeron, Mark Tyra, Jerome LaRosa, Svetlana Nour, M Andriamirado, A.B. Balantekin, H.R. Band, C.D. Bass, D. Berish, N.S. Bowden, J.P. Brodsky, C.D. Bryan, T. Classen, A.J. Conant, G. Deichert, M.V. Diwan, M.J. Dolinski, A. Erickson, B.T. Foust, J.K. Gaison, A. Galindo-Uribarri, C.E. Gilbert, B.W. Goddard, B.T. Hackett, S. Hans, A.B. Hansell, K.M. Heeger, D.E. Jaffe, X. Ji, D.C. Jones, O. Kyzylova, C.E. Lane, T.J. Langford, B.R. Littlejohn, X. Lu, J. Maricic, M.P. Mendenhall, A.M. Meyer, R. Milincic, I. Mitchell, P.E. Mueller, J. Napolitano, C. Nave, R. Neilson, J.A. Nikkel, D. Norcini, J.L. Palomino, D.A. Pushin, X. Qian, E. Romero-Romero, R. Rosero, P.T. Surukuchi, R.L. Varner, D. Venegas-Vargas, P.B. Weatherly, C. White, J. Wilhelmi, A. Woolverton, M. Yeh, A. Zhang, C. Zhang, X. Zhang
If dark matter has mass lower than around 1 GeV, it will not impart enough energy to cause detectable nuclear recoils in many direct-detection experiments
Created October 3, 2019, Updated February 10, 2025