FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1882034605> ?p ?o ?g. }

• W1882034605 abstract "We determine the prospects for finding dark matter at the Tevatron and LHC through the production of exotic fourth-generation mirror quarks ${T}^{ensuremath{'}}$ that decay through ${T}^{ensuremath{'}}ensuremath{rightarrow}tX$, where $X$ is dark matter. The resulting signal of $toverline{t}+{mathrm{Eensuremath{llap{not;}}}}_{T}$ has not previously been considered in searches for fourth-generation quarks, but there are both general and specific dark matter motivations for this signal, and with slight modifications, this analysis applies to any scenario where invisible particles are produced in association with top quarks. Current direct and indirect bounds on such exotic quarks restrict their masses to be between 300 and 600 GeV, and the dark matter's mass may be anywhere below ${m}_{{T}^{ensuremath{'}}}$. We simulate the signal and main backgrounds with MadGraph/MadEvent-Pythia-PGS4. For the Tevatron, we find that an integrated luminosity of $20text{ }text{ }{mathrm{fb}}^{ensuremath{-}1}$ will allow $3ensuremath{sigma}$ discovery up to ${m}_{{T}^{ensuremath{'}}}=400text{ }text{ }mathrm{GeV}$ and 95% exclusion up to ${m}_{{T}^{ensuremath{'}}}=455text{ }text{ }mathrm{GeV}$. For the 10 TeV LHC with $300text{ }text{ }{mathrm{pb}}^{ensuremath{-}1}$, the discovery and exclusion sensitivities rise to 490 GeV and 600 GeV. These scenarios are therefore among the most promising for dark matter at colliders. Perhaps most interestingly, we find that dark matter models that can explain results from the DAMA, CDMS, and CoGeNT collaborations can be tested with high statistical significance using data already collected at the Tevatron and have extraordinarily promising implications for early runs of the LHC." @default.
• W1882034605 created "2016-06-24" @default.
• W1882034605 creator A5010493054 @default.
• W1882034605 creator A5014047994 @default.
• W1882034605 creator A5050787710 @default.
• W1882034605 creator A5080030068 @default.
• W1882034605 date "2010-06-17" @default.
• W1882034605 modified "2023-10-05" @default.
• W1882034605 title "Dark matter-motivated searches for exotic fourth-generation mirror quarks in Tevatron and early LHC data" @default.
• W1882034605 cites W1513847875 @default.
• W1882034605 cites W1539212645 @default.
• W1882034605 cites W1557310419 @default.
• W1882034605 cites W1677693 @default.
• W1882034605 cites W1839713160 @default.
• W1882034605 cites W1969909363 @default.
• W1882034605 cites W1980573344 @default.
• W1882034605 cites W1981386653 @default.
• W1882034605 cites W1981955221 @default.
• W1882034605 cites W1990449676 @default.
• W1882034605 cites W1990876092 @default.
• W1882034605 cites W1996889746 @default.
• W1882034605 cites W2001560451 @default.
• W1882034605 cites W2001780075 @default.
• W1882034605 cites W2006473173 @default.
• W1882034605 cites W2006528212 @default.
• W1882034605 cites W2008832100 @default.
• W1882034605 cites W2012164873 @default.
• W1882034605 cites W2016207935 @default.
• W1882034605 cites W201997629 @default.
• W1882034605 cites W2022456258 @default.
• W1882034605 cites W2028545023 @default.
• W1882034605 cites W2038748210 @default.
• W1882034605 cites W2039276976 @default.
• W1882034605 cites W2043581053 @default.
• W1882034605 cites W2047402856 @default.
• W1882034605 cites W2047664995 @default.
• W1882034605 cites W2063398773 @default.
• W1882034605 cites W2063465519 @default.
• W1882034605 cites W2071929640 @default.
• W1882034605 cites W2073616263 @default.
• W1882034605 cites W2075816320 @default.
• W1882034605 cites W2078593377 @default.
• W1882034605 cites W2082595344 @default.
• W1882034605 cites W2093069506 @default.
• W1882034605 cites W2093741005 @default.
• W1882034605 cites W2101392458 @default.
• W1882034605 cites W2106662935 @default.
• W1882034605 cites W2114987342 @default.
• W1882034605 cites W2118121119 @default.
• W1882034605 cites W2119492067 @default.
• W1882034605 cites W2124464017 @default.
• W1882034605 cites W2128179456 @default.
• W1882034605 cites W2128730339 @default.
• W1882034605 cites W2129101324 @default.
• W1882034605 cites W2133761278 @default.
• W1882034605 cites W2135748922 @default.
• W1882034605 cites W2148144009 @default.
• W1882034605 cites W2155591485 @default.
• W1882034605 cites W2161075311 @default.
• W1882034605 cites W2258584306 @default.
• W1882034605 cites W2270901284 @default.
• W1882034605 cites W2530254136 @default.
• W1882034605 cites W2963598458 @default.
• W1882034605 cites W3023468824 @default.
• W1882034605 cites W3098678441 @default.
• W1882034605 cites W3099247730 @default.
• W1882034605 cites W3099673264 @default.
• W1882034605 cites W3099678564 @default.
• W1882034605 cites W3100824667 @default.
• W1882034605 cites W3101764270 @default.
• W1882034605 cites W3102873965 @default.
• W1882034605 cites W3102930836 @default.
• W1882034605 cites W3104130143 @default.
• W1882034605 cites W3104412157 @default.
• W1882034605 cites W3104841526 @default.
• W1882034605 cites W3105438058 @default.
• W1882034605 cites W3105446304 @default.
• W1882034605 cites W3105919334 @default.
• W1882034605 cites W3123750486 @default.
• W1882034605 cites W61345581 @default.
• W1882034605 doi "https://doi.org/10.1103/physrevd.81.114027" @default.
• W1882034605 hasPublicationYear "2010" @default.
• W1882034605 type Work @default.
• W1882034605 sameAs 1882034605 @default.
• W1882034605 citedByCount "46" @default.
• W1882034605 countsByYear W18820346052012 @default.
• W1882034605 countsByYear W18820346052013 @default.
• W1882034605 countsByYear W18820346052014 @default.
• W1882034605 countsByYear W18820346052015 @default.
• W1882034605 countsByYear W18820346052016 @default.
• W1882034605 countsByYear W18820346052017 @default.
• W1882034605 countsByYear W18820346052020 @default.
• W1882034605 countsByYear W18820346052022 @default.
• W1882034605 countsByYear W18820346052023 @default.
• W1882034605 crossrefType "journal-article" @default.
• W1882034605 hasAuthorship W1882034605A5010493054 @default.
• W1882034605 hasAuthorship W1882034605A5014047994 @default.
• W1882034605 hasAuthorship W1882034605A5050787710 @default.
• W1882034605 hasAuthorship W1882034605A5080030068 @default.
• W1882034605 hasBestOaLocation W18820346052 @default.

• next