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• W2895980914 abstract "Dark photons (DP) are interesting as potential mediators between the dark matter (DM) sector and the fields of the Standard Model (SM). The interaction of the DP, described by a broken $U(1)_D$ gauge symmetry, with the SM is usually generated at the one-loop level via kinetic mixing through the existence of portal matter (PM), here assumed to be fermionic, which carries both a dark charge as well as a SM $U(1)_Y$ hypercharge. For theoretical consistency, as well as for many phenomenological reasons, this PM must be vector-like with respect to the SM and dark gauge groups and, in particular, is shown to be allowed only to transform as vector-like copies of the usual SM fields. The dark Higgs that is responsible for the breaking of $U(1)_D$ can then generate a mixing between the PM and SM fields with the same electric charge thus altering the DP interactions with (at least some of) the SM fields and also providing a path for the PM fields to decay. In this paper we briefly explore the phenomenology of some specific simple models of this PM including, for the case where the PM is leptonic in nature, their potential impact on experiments probing low energy parity-violation and the g-2 of the muon. In the case of color-triplet, bottom quark-like PM, their direct pair- and single-production at the LHC is shown to be observable in final states that include missing $E_T$ and/or very highly boosted lepton-jets together with pairs of high $p_T$ b-jets that can be used to trigger on such events. These signatures are quite distinct from those usually employed in the search for vector-like quarks at the LHC and, furthermore, we demonstrate that the conventional signal channels for vector-like quarks involving the SM Higgs and gauge fields are essentially closed in the case of PM." @default.
• W2895980914 created "2018-10-26" @default.
• W2895980914 creator A5029905577 @default.
• W2895980914 date "2019-06-18" @default.
• W2895980914 modified "2023-10-05" @default.
• W2895980914 title "Kinetic mixing and portal matter phenomenology" @default.
• W2895980914 cites W1689327406 @default.
• W2895980914 cites W1895221770 @default.
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• W2895980914 cites W1964503396 @default.
• W2895980914 cites W1987435915 @default.
• W2895980914 cites W1988439317 @default.
• W2895980914 cites W2009407387 @default.
• W2895980914 cites W2020885902 @default.
• W2895980914 cites W2022778241 @default.
• W2895980914 cites W2030684353 @default.
• W2895980914 cites W2031026718 @default.
• W2895980914 cites W2035247566 @default.
• W2895980914 cites W2043653474 @default.
• W2895980914 cites W2053366165 @default.
• W2895980914 cites W2063701107 @default.
• W2895980914 cites W2064555570 @default.
• W2895980914 cites W2068026536 @default.
• W2895980914 cites W2075093571 @default.
• W2895980914 cites W2081514725 @default.
• W2895980914 cites W2100678356 @default.
• W2895980914 cites W2101946481 @default.
• W2895980914 cites W2106091945 @default.
• W2895980914 cites W2107925921 @default.
• W2895980914 cites W2109886938 @default.
• W2895980914 cites W2118050609 @default.
• W2895980914 cites W2122360507 @default.
• W2895980914 cites W2124142696 @default.
• W2895980914 cites W2140902438 @default.
• W2895980914 cites W2146291923 @default.
• W2895980914 cites W2153953405 @default.
• W2895980914 cites W2158557180 @default.
• W2895980914 cites W2163186315 @default.
• W2895980914 cites W2163881764 @default.
• W2895980914 cites W2165093219 @default.
• W2895980914 cites W2168387489 @default.
• W2895980914 cites W2170362449 @default.
• W2895980914 cites W2171592884 @default.
• W2895980914 cites W2266968426 @default.
• W2895980914 cites W2321547729 @default.
• W2895980914 cites W2510008745 @default.
• W2895980914 cites W2547940623 @default.
• W2895980914 cites W2588359325 @default.
• W2895980914 cites W2593779016 @default.
• W2895980914 cites W2597602507 @default.
• W2895980914 cites W2602969550 @default.
• W2895980914 cites W2605078543 @default.
• W2895980914 cites W2606304933 @default.
• W2895980914 cites W2608787054 @default.
• W2895980914 cites W2619445463 @default.
• W2895980914 cites W2742211086 @default.
• W2895980914 cites W2751798936 @default.
• W2895980914 cites W2767782935 @default.
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• W2895980914 cites W2883192089 @default.
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• W2895980914 cites W2910729192 @default.
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• W2895980914 cites W3105575239 @default.
• W2895980914 cites W3105619082 @default.
• W2895980914 cites W3124210849 @default.
• W2895980914 cites W3126051712 @default.
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• W2895980914 doi "https://doi.org/10.1103/physrevd.99.115024" @default.
• W2895980914 hasPublicationYear "2019" @default.
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