We constrain, from the observed properties of diffuse interstellar clouds, the interactions of halo particles with atomic hydrogen.
DOI:https://doi.org/10.1103/PhysRevLett.65.957
©1990 American Physical Society
R. Sekhar Chivukula, Andrew G. Cohen, and Savas Dimopoulos
Terry P. Walker
Vol. 65, Iss. 8 — 20 August 1990
Sign up to receive regular email alerts from Physical Review Letters