The Open UniversitySkip to content
 

A numerical model of ion implantation into presolar grains

Verchovsky, A.V.; Wright, I.P.; Fisenko, A.V. and Pillinger, C.T. (2001). A numerical model of ion implantation into presolar grains. Nuclear Physics A, 688(1-2) 106C-109C.

DOI (Digital Object Identifier) Link: http://dx.doi.org/10.1016/S0375-9474(01)00678-9
Google Scholar: Look up in Google Scholar

Abstract

Pre-solar grains such as diamond and silicon carbide (found in primitive chondritic meteorites), contain isotopically anomalous noble gases. There are two ways that these could have been incorporated into the grains: direct assimilation during grain formation and growth, or subsequent addition after the grains had formed. Herein we investigate the latter possibililty and explore the role of ion implementation within the interstellar medium (i.e. into pre-existing grains distributed in free space). Numerical models are derived to address the issue of how ion implantation would affect the grain population.

Item Type: Journal Article
ISSN: 0375-9474
Academic Unit/Department: Science > Physical Sciences
Interdisciplinary Research Centre: Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)
Item ID: 3417
Depositing User: Users 6044 not found.
Date Deposited: 29 Nov 2006
Last Modified: 02 Dec 2010 19:49
URI: http://oro.open.ac.uk/id/eprint/3417
Share this page:

Actions (login may be required)

View Item
Report issue / request change

Policies | Disclaimer

© The Open University   + 44 (0)870 333 4340   general-enquiries@open.ac.uk