Damage to Relativistic Interstellar Spacecraft by ISM Impact Gas Accumulation
Jon Drobny, Alexander N. Cohen, Davide Curreli, Philip Lubin, Maria G., Pelizzo, Maxim Umansky

TL;DR
This paper investigates how impacts from interstellar medium particles cause gas accumulation and material damage on relativistic spacecraft, affecting their integrity and suggesting mitigation strategies.
Contribution
It introduces a new model for predicting blistering thresholds due to gas implantation from ISM impacts at relativistic speeds.
Findings
Gas implantation leads to bubble formation and material erosion.
Near-surface gas distribution differs from empirical blistering models.
Proposes mitigation strategies for spacecraft durability.
Abstract
As part of the NASA Starlight collaboration, we look at the implications of radiation effects from impacts with the interstellar medium (ISM) on a directed energy driven relativistic spacecraft. The spacecraft experiences a stream of MeV/nucleon impacts along the forward edge primarily from hydrogen and helium nuclei. The accumulation of implanted slowly diffusing gas atoms in solids drives damage through the meso-scale processes of bubble formation, blistering, and exfoliation. This results in macroscopic changes to material properties and, in the cases of blistering and exfoliation, material erosion via blister rupture and delamination. Relativistic hydrogen and helium at constant velocity will stop in the material at a similar depth, as predicted by Bethe-Bloch stopping and subsequent simulations of the implantation distribution, leading to a mixed hydrogen and helium system similar…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
