Michael CherryCherry

Roy P. Daniels Professor of Physics

Ph.D., 1978 - University of Chicago

Louisiana State University
Department of Physics & Astronomy
343-D Nicholson Hall, Tower Dr.
Baton Rouge, LA 70803-4001
(225) 578-8591-Office

Personal Webpage

Research Interests

Space Science / High Energy Astrophysics

High energy astrophysics deals with the radiation produced by energetic particles in space, their astrophysical sources, and the acceleration mechanisms that produce the very high energy particles. We observe cosmic ray protons and nuclei at earth with energies orders of magnitude higher than the proton rest mass. Our previous JACEE balloon measurements show no evidence for the expected drop-off in the proton-helium spectra due to acceleration by supernova shocks. The ATIC collaboration, in addition to measuring elemental spectra, reported an anomalous enhancement in the electron flux below a TeV. Our LSU group is now involved in the operation of the CALET (CALorimetric Electron Telescope) experiment on the International Space Station,  to provide a definitive measurement of the high energy electron spectrum.

Since charged cosmic ray particles are randomized in direction by the galaxy's magnetic field, however, they do not come in straight lines from their sources. Hard x-rays and gamma rays (10 keV - 40 MeV) provide direct information about the high energy sources. The Gamma ray Burst Monitor (GBM) on the Fermi satellite is being used to monitor the hard x-ray sky, and has detected an unexpected time dependence of the flux from the Crab Nebula. Our group is involved in analyzing the GBM and earlier CGRO/BATSE earth occultation data. GBM has observed flaring activity from the blazars M421 and M501, Sco X-1, Cygnus X-1, and the transient X-ray pulsar system V0332+53.

We are operating a ground-based array that has detected Terrestrial Gamma ray Flashes (TGFs), bursts of gamma rays associated with nearby lightning storms, and have installed two large scintillator arrays in Puerto Rico and Panama in locations where the lightning intensity is a good deal higher than in Louisiana.

Finally, we are developing the transition radiation detectors to be used to identify protons, kaons, and pions at TeV energies for a proposed CERN experiment to measure high energy cross sections in the far forward region.

Current and Select Publications

"First Results from Fermi GBM Earth Occultation Monitoring: Observations of Soft Gamma-Ray Sources Above 100 keV", G.L. Case et al.,Astrophysical J. 729, 105 (2011). Article.

“When A Standard Candle Flickers”, C.A. Wilson-Hodge et al., Astrophysical J. Letters 727, L40 (2011). Article. 

“Characteristic Count Rate Profiles for a Rotating Modulator Gamma-Ray Imager”, B.S. Budden et al., Astrophys. and Space Sci. 334, 61 (2011). Article.

“CALET: A Calorimeter-based Orbital Observatory for High Energy Astroparticle Physics”, P.S. Marrocchesi for the CALET Collaboration, Nucl. Instrum. Meth. in Phys. Res. A, 692, 240 (2012). Article

“Measuring the Lorentz Factors of Energetic Particles with Transition Radiation”, M.L. Cherry, Nucl. Instrum. Meth. in Phys. Res. A 706, 39 (2013). Article.

“Observation of Gamma Rays at Ground Level Associated with Nearby Thunderstorms", R. Ringuette et al., J. Geophysical Res: Space Phys. 118, 7841 (2013). Article.

“Kepler K2 Observations of Sco X-1: Orbital Modulations and Correlations with Fermi GBM and MAXI", R.I. Hynes et al., MNRAS 459, 3596 (2016). Article.  

"Observations of V0332+53 during the 2015 Outburst using Fermi/GBM, MAXI, Swift, and INTEGRA". Z.Baum et al; MNRAS 467, 4424 (2017). Article.  

 “CALET Upper Limits on X-Ray and Gamma-Ray Counterparts of GW 151226”, O. Adriani et al., Astrophysical Journal Letters, 829, L20 (2016). Article.

“Energy Spectrum of Cosmic Ray Electron + Positron from 10 GeV to 3 TeV Observed with the Calorimetric Electron Telescope on the International Space Station”, O. Adriani et al., Phys. Rev. Lett. 119, 181101 (2017). Article

“Multi-Messenger Observations of a Binary Neutron Star Merger”, B.P. Abbott et al. (LIGO Scientific Collaboration, VIRGO Collaboration, and Partner Astronomy Groups), Astrophys. J. Lett. 848:L12 (2017). Article

“High Statistics Measurement of Cosmic-ray Electron and Positron Spectrum from 11 GeV to 4.8 TeV with the Calorimetric Electron Telescope on the International Space Station”, Y. Asaoka et al. , Phys. Rev. Lett. 120, 261102 (2018); Article

“Characteristics and Performance of the Calorimetric Electron Telescope (CALET) Calorimeter for Gamma-Ray Observations”, N. Cannady et al., Astrophys. J. Suppl. 238:5 (2018); Article

“Search for GeV Gamma-ray Counterparts of Gravitational Wave Events byCALET”, O. Adriani et al., Astrophys. J. 863 (2018); Article

“First Measurements of the Spectral and Angular Distribution of Transition Radiation Using a Silicon Pixel Sensor on a Timepix3 Chip”, E. J. Schioppa et al., Nucl. Instrum. Methods A, to be published (2019); Article

“Identification of particles with Lorentz factor up to 104 with Transition Radiation Detectors Based on Micro-strip Silicon Detectors”, J. Alozy et al., Nucl. Instrum. Meth. A 927, 1 (2019); Article

“Direct Measurement of the Cosmic-Ray Proton Spectrum from 50 GeV to 10 TeV with the Calorimetric Electron Telescope on the International Space Station”, O. Adriani et al., Phys. Rev. Lett. 122, 181102 (2019); Article