Measurement of Cosmic Ray Lithium Isotopes Using the Alpha Magnetic Spectrometer

The study of cosmic rays and their properties provides insight into the origins of our universe and is a unique lens on the nuclear physics of the cosmos. The identification of cosmic ray isotopes poses a particular challenge, as it requires the measurement of multiple observables to a high degree of accuracy for the deduction of nuclear mass. Using the unique detection capabilities of the Alpha Magnetic Spectrometer (AMS), the isotope fluxes of cosmic ray lithium in the rigidity range of 1.92 to 25 GV are presented. This work is based on 0.97 million ⁶Li and 1.04 million ⁷Li nuclei collected by the AMS over a 12.5 year period, and improves the error and extent of existing measurements by a factor of 10. These results lead to the conclusion that there is no sizable primary component in cosmic ray ⁷Li. The improvements to the AMS velocity measurement establishes the groundwork for future cosmic ray isotope measurements.

Name thesis:degree_name

Doctoral

Department dc:contributor.department

Massachusetts Institute of Technology. Department of Physics

Grantor dc:publisher

Massachusetts Institute of Technology

Year dc:date.issued

2025

Author dc:creator

• LaVecchia, Gianni

Advisor dc:contributor.advisor

• Ting, Samuel

Statement dc:rights

• In Copyright - Educational Use Permitted
• Copyright retained by author(s)

Licence dc:rights.uri

• https://rightsstatements.org/page/InC-EDU/1.0/

Handle dc:identifier.uri

https://hdl.handle.net/1721.1/164154

OAI identifier oai:identifier

oai:dspace.mit.edu:1721.1/164154