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A noise model for the LISA gravitational wave detector

Grant number: 07/07332-8
Support type:Scholarships in Brazil - Scientific Initiation
Effective date (Start): February 01, 2008
Effective date (End): January 31, 2009
Field of knowledge:Physical Sciences and Mathematics - Physics - Elementary Particle Physics and Fields
Principal Investigator:Carlos Frajuca
Grantee:Juliana Schell
Home Institution: Centro Federal de Educação Tecnológica de São Paulo. Ministério da Educação (Brasil). São Paulo , SP, Brazil
Associated research grant:06/56041-3 - New physics from space: gravitational waves, AP.TEM


LISA is a project of an interferometric gravitational wave detector to be assembled in space, so the abbreviature LISA means Laser Interferometer Space Antenna. The LISA function is to find wavelength fluctuations in the sides of an equilateral triangle with side-length of 5x106km shaped by spaceships in each vertex of the triangle. The goal of this work is to re-elaborate a noise model for the LISA, discovering how the detector sensibility changes with variation in each detector characteristic and suggesting possible modifications in the actual project.