000003932 001__ 3932
000003932 005__ 20190128111216.0
000003932 0247_ $$2DOI$$a10.1109/CPEM.2018.8500921
000003932 037__ $$aSCART-2019-0074
000003932 088__ $$aINSPEC Accession Number: 18193266
000003932 100__ $$aBertrand, Bruno
000003932 245__ $$aA Model of Massive Electromagnetism for the Detection of Topological Dark Matter Through GNSS Networks
000003932 260__ $$c2018
000003932 520__ $$aWe formulate a new theoretical model which paves the way for methods of detection of particular types of dark matter using GNSS networks. Our model consists in a (topologically) massive version of Maxwell theory in a medium which admits topological defect solutions. Hence it describes hypothetical dark matter consisting in Earth-sized structures like monopoles, vortices or domain walls which could induce disturbances in the GNSS networks. In the future our model will then be constrained by GNSS measurements.
000003932 594__ $$aNO
000003932 6531_ $$aDark matter
000003932 6531_ $$aElectromagnetic measurements
000003932 6531_ $$aElectromagnetic propagation
000003932 6531_ $$aGlobal Navigation Satellite System
000003932 6531_ $$aTopological defects
000003932 700__ $$aDefraigne, Pascale
000003932 773__ $$p2018 Conference on Precision Electromagnetic Measurements (CPEM 2018)$$y2018
000003932 8560_ $$fbruno.bertrand@observatoire.be
000003932 85642 $$ahttp://ieeexplore.ieee.org/stamp/stamp.jsp?tp=&arnumber=8500921&isnumber=8500784
000003932 905__ $$apublished in
000003932 980__ $$aREFERD