Neil Lambert | |
---|---|
Alma mater | University of Toronto University of Cambridge |
Known for | Bagger–Lambert–Gustavsson action |
Scientific career | |
Fields | Theoretical physics |
Institutions | King's College London |
Neil Lambert is a Professor in theoretical physics at King's College London. His research is primarily concerned with supersymmetry, string theory and M-theory. [1]
Lambert graduated from University of Toronto with BSc in mathematics and physics in 1992. He did his graduate studies at Cambridge University.
He was also a staff physicist at CERN from 2010 to 2013. [1]
BSc, University of Toronto (Graduated in 1992). [1]
PhD, Cambridge University (Advisor: Paul Townsend. Graduated in 1996). [1]
From 2000 to 2005 he held a PPARC Advanced Fellowship at King's College London, and later was given a lectureship and later a chair in 2009. He has also held post-doctoral positions at École normale supérieure (Paris) and Rutgers University. From 2010 to 2013 he was a staff physicist at CERN. [1] He also holds the post of honorary advisor at BMUCO, which is a university student-led science organisation. [2]
Supersymmetry is a theoretical framework in physics that suggests the existence of a symmetry between particles with integer spin (bosons) and particles with half-integer spin (fermions). It proposes that for every known particle, there exists a partner particle with different spin properties. There have been multiple experiments on supersymmetry that have failed to provide evidence that it exists in nature. If evidence is found, supersymmetry could help explain certain phenomena, such as the nature of dark matter and the hierarchy problem in particle physics.
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H͂
, is the superpartner of the Higgs field. A higgsino is a Dirac fermionic field with spin 1⁄2 and it refers to a weak isodoublet with hypercharge half under the Standard Model gauge symmetries. After electroweak symmetry breaking higgsino fields linearly mix with U(1) and SU(2) gauginos leading to four neutralinos and two charginos that refer to physical particles. While the two charginos are charged Dirac fermions, the neutralinos are electrically neutral Majorana fermions. In an R-parity-conserving version of the Minimal Supersymmetric Standard Model, the lightest neutralino typically becomes the lightest supersymmetric particle (LSP). The LSP is a particle physics candidate for the dark matter of the universe since it cannot decay to particles with lighter mass. A neutralino LSP, depending on its composition can be bino, wino or higgsino dominated in nature and can have different zones of mass values in order to satisfy the estimated dark matter relic density. Commonly, a higgsino dominated LSP is often referred as a higgsino, in spite of the fact that a higgsino is not a physical state in the true sense.
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