Matches in SemOpenAlex for { <https://semopenalex.org/work/W2150150908> ?p ?o ?g. }
- W2150150908 abstract "Motivated by the dark matter and the baryon asymmetry problems, we analyse a complex singlet extension of the Standard Model (SM) with a Z2 symmetry (which provides a dark matter candidate). After a detailed two-loop calculation of the renormalization group equations for the new scalar sector, we study the radiative stability of the model up to a high energy scale (with the constraint that the 126 GeV Higgs boson found at the LHC is in the spectrum) and find it requires the existence of a new scalar state mixing with the Higgs with a mass larger than 140 GeV. This bound is not very sensitive to the cut-off scale as long as the latter is larger than 10^10 GeV. We then include all experimental and observational constraints/measurements from collider data, dark matter direct detection experiments and from the Planck satellite and in addition force stability at least up to the GUT scale, to find that the lower bound is raised to about 170 GeV, while the dark matter particle must be heavier than about 50 GeV." @default.
- W2150150908 created "2016-06-24" @default.
- W2150150908 creator A5020154569 @default.
- W2150150908 creator A5023633796 @default.
- W2150150908 creator A5030249425 @default.
- W2150150908 creator A5055444470 @default.
- W2150150908 date "2015-07-16" @default.
- W2150150908 modified "2023-10-14" @default.
- W2150150908 title "Two-loop stability of a complex singlet extended standard model" @default.
- W2150150908 cites W1505073703 @default.
- W2150150908 cites W1567660396 @default.
- W2150150908 cites W1569986947 @default.
- W2150150908 cites W1889411329 @default.
- W2150150908 cites W1968452157 @default.
- W2150150908 cites W1968756892 @default.
- W2150150908 cites W1974897902 @default.
- W2150150908 cites W1979771157 @default.
- W2150150908 cites W1981563312 @default.
- W2150150908 cites W1983178413 @default.
- W2150150908 cites W1983768061 @default.
- W2150150908 cites W1988820440 @default.
- W2150150908 cites W1993895680 @default.
- W2150150908 cites W1996218638 @default.
- W2150150908 cites W2005952444 @default.
- W2150150908 cites W2010410835 @default.
- W2150150908 cites W2011238680 @default.
- W2150150908 cites W2011547671 @default.
- W2150150908 cites W2012628526 @default.
- W2150150908 cites W2024670199 @default.
- W2150150908 cites W2027413505 @default.
- W2150150908 cites W2034391218 @default.
- W2150150908 cites W2034883041 @default.
- W2150150908 cites W2038352995 @default.
- W2150150908 cites W2040712769 @default.
- W2150150908 cites W2041000749 @default.
- W2150150908 cites W2042260934 @default.
- W2150150908 cites W2048393950 @default.
- W2150150908 cites W2053975209 @default.
- W2150150908 cites W2054245752 @default.
- W2150150908 cites W2065045130 @default.
- W2150150908 cites W2065787695 @default.
- W2150150908 cites W2067260962 @default.
- W2150150908 cites W2075040906 @default.
- W2150150908 cites W2075093571 @default.
- W2150150908 cites W2080033597 @default.
- W2150150908 cites W2085107687 @default.
- W2150150908 cites W2097455345 @default.
- W2150150908 cites W2102418840 @default.
- W2150150908 cites W2111808546 @default.
- W2150150908 cites W2115990939 @default.
- W2150150908 cites W2116125044 @default.
- W2150150908 cites W2121559823 @default.
- W2150150908 cites W2131587105 @default.
- W2150150908 cites W2136821211 @default.
- W2150150908 cites W2139937287 @default.
- W2150150908 cites W2142433810 @default.
- W2150150908 cites W2145202687 @default.
- W2150150908 cites W2149695318 @default.
- W2150150908 cites W2152171676 @default.
- W2150150908 cites W2153433018 @default.
- W2150150908 cites W2154380446 @default.
- W2150150908 cites W2156207194 @default.
- W2150150908 cites W2159266306 @default.
- W2150150908 cites W2160723489 @default.
- W2150150908 cites W2163668057 @default.
- W2150150908 cites W2165679618 @default.
- W2150150908 cites W2167803448 @default.
- W2150150908 cites W2168134144 @default.
- W2150150908 cites W2171932407 @default.
- W2150150908 cites W2172978159 @default.
- W2150150908 cites W2174087929 @default.
- W2150150908 cites W2180262730 @default.
- W2150150908 cites W2594808321 @default.
- W2150150908 cites W3100514957 @default.
- W2150150908 cites W3100931324 @default.
- W2150150908 cites W3101238927 @default.
- W2150150908 cites W3101661011 @default.
- W2150150908 cites W3101821865 @default.
- W2150150908 cites W3102876032 @default.
- W2150150908 cites W3103395790 @default.
- W2150150908 cites W3103461829 @default.
- W2150150908 cites W3103706258 @default.
- W2150150908 cites W3104096922 @default.
- W2150150908 cites W3104728558 @default.
- W2150150908 cites W3105872726 @default.
- W2150150908 cites W4250636715 @default.
- W2150150908 cites W4255860707 @default.
- W2150150908 doi "https://doi.org/10.1103/physrevd.92.025024" @default.
- W2150150908 hasPublicationYear "2015" @default.
- W2150150908 type Work @default.
- W2150150908 sameAs 2150150908 @default.
- W2150150908 citedByCount "51" @default.
- W2150150908 countsByYear W21501509082015 @default.
- W2150150908 countsByYear W21501509082016 @default.
- W2150150908 countsByYear W21501509082017 @default.
- W2150150908 countsByYear W21501509082018 @default.
- W2150150908 countsByYear W21501509082019 @default.
- W2150150908 countsByYear W21501509082020 @default.
- W2150150908 countsByYear W21501509082021 @default.
- W2150150908 countsByYear W21501509082022 @default.