FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1997364667> ?p ?o ?g. }

• W1997364667 abstract "that would exploit the existing Accumulator and Debuncher rings to generate the required characteristics of the primary proton beam. The proposal requires only modest modifications to the accelerator complex after including those already planned for the NOvA experiment, with which this experiment would be fully compatible. The search for lepton flavor violation (LFV) has long played an important role in the evolution of our understanding of electroweak interactions. The neutrinoless conversion of a muon to an electron in the field of a nucleus is a particularly interesting example of an LFV process involving charged leptons. In the Standard Model, such conversions would take place via loop diagrams involving virtual neutrino mixing, at a rate far below the threshold of any currently conceivable experiment. Indeed, any detectable signal would be a definite indication, albeit indirect, of new dynamics at multi-TeV energy scales. Enhanced rate for this process is an almost universal feature of beyond the Standard Model physics, and the fact that such a process has not been observed has constrained or eliminated many models [1]. While it is widely believed that new physics will appear at LHC energies, the LHC is not well-equipped to study LFV directly. An often-quoted example is in the case of supersymmetry. The LHC will probe slepton masses, but it cannot compete with muon decay experiments in constraining the slepton mixing angles. Sensitive searches for rare or forbidden leptonic and semi-leptonic LFV processes, especially those involving charged leptons, are essential for the comprehensive characterization of new high energy physics. While there are several potential reactions that can be used to probe LFV, muon to electron conversion has the remarkable feature that it does not require the coincidence of two final-state particles. The spectacular signature is a single conversion electron of well-defined energy, separated from most of the sources of background. As a result, very high muon data rates can be handled and an unusually sensitive search for LFV becomes feasible. Indeed, at the level of sensitivity discussed below, a large class of supersymmetric models would predict 100's of conversion events. Additionally, compositeness and Z{prime} models would be probed at the multi-TeV scale in a manner complementary to direct LHC searches. Lepto-quarks would be probed at the 3000 TeV scale. Muon to electron conversion is therefore sensitive to many new physics scenarios at energy scales that cannot be probed by direct searches using other foreseeable accelerators." @default.
• W1997364667 created "2016-06-24" @default.
• W1997364667 creator A5000028915 @default.
• W1997364667 creator A5000098804 @default.
• W1997364667 creator A5000173022 @default.
• W1997364667 creator A5000188065 @default.
• W1997364667 creator A5000596772 @default.
• W1997364667 creator A5002525140 @default.
• W1997364667 creator A5003499284 @default.
• W1997364667 creator A5006307308 @default.
• W1997364667 creator A5009092217 @default.
• W1997364667 creator A5010319650 @default.
• W1997364667 creator A5011447117 @default.
• W1997364667 creator A5014351060 @default.
• W1997364667 creator A5015688454 @default.
• W1997364667 creator A5017971531 @default.
• W1997364667 creator A5018872449 @default.
• W1997364667 creator A5019825165 @default.
• W1997364667 creator A5019831101 @default.
• W1997364667 creator A5020534545 @default.
• W1997364667 creator A5020899301 @default.
• W1997364667 creator A5021635558 @default.
• W1997364667 creator A5022042272 @default.
• W1997364667 creator A5022927417 @default.
• W1997364667 creator A5025484280 @default.
• W1997364667 creator A5026167700 @default.
• W1997364667 creator A5028306374 @default.
• W1997364667 creator A5028539059 @default.
• W1997364667 creator A5029062001 @default.
• W1997364667 creator A5029428493 @default.
• W1997364667 creator A5030465973 @default.
• W1997364667 creator A5032436815 @default.
• W1997364667 creator A5032700123 @default.
• W1997364667 creator A5035791032 @default.
• W1997364667 creator A5037910508 @default.
• W1997364667 creator A5041252363 @default.
• W1997364667 creator A5046315734 @default.
• W1997364667 creator A5046595499 @default.
• W1997364667 creator A5047783841 @default.
• W1997364667 creator A5048720394 @default.
• W1997364667 creator A5050889155 @default.
• W1997364667 creator A5053335435 @default.
• W1997364667 creator A5053982613 @default.
• W1997364667 creator A5054855688 @default.
• W1997364667 creator A5055829061 @default.
• W1997364667 creator A5056576647 @default.
• W1997364667 creator A5057244690 @default.
• W1997364667 creator A5058359050 @default.
• W1997364667 creator A5061068837 @default.
• W1997364667 creator A5062070398 @default.
• W1997364667 creator A5063161579 @default.
• W1997364667 creator A5063781733 @default.
• W1997364667 creator A5068647296 @default.
• W1997364667 creator A5069974508 @default.
• W1997364667 creator A5071702251 @default.
• W1997364667 creator A5072582288 @default.
• W1997364667 creator A5075559240 @default.
• W1997364667 creator A5076157676 @default.
• W1997364667 creator A5076284541 @default.
• W1997364667 creator A5077555409 @default.
• W1997364667 creator A5080780148 @default.
• W1997364667 creator A5081247179 @default.
• W1997364667 creator A5084280248 @default.
• W1997364667 creator A5084301323 @default.
• W1997364667 creator A5086556132 @default.
• W1997364667 date "1997-09-01" @default.
• W1997364667 modified "2023-09-25" @default.
• W1997364667 title "BTeV: An Expression of interest for a heavy quark program at C0" @default.
• W1997364667 doi "https://doi.org/10.2172/1156364" @default.
• W1997364667 hasPublicationYear "1997" @default.
• W1997364667 type Work @default.
• W1997364667 sameAs 1997364667 @default.
• W1997364667 citedByCount "7" @default.
• W1997364667 countsByYear W19973646672016 @default.
• W1997364667 crossrefType "report" @default.
• W1997364667 hasAuthorship W1997364667A5000028915 @default.
• W1997364667 hasAuthorship W1997364667A5000098804 @default.
• W1997364667 hasAuthorship W1997364667A5000173022 @default.
• W1997364667 hasAuthorship W1997364667A5000188065 @default.
• W1997364667 hasAuthorship W1997364667A5000596772 @default.
• W1997364667 hasAuthorship W1997364667A5002525140 @default.
• W1997364667 hasAuthorship W1997364667A5003499284 @default.
• W1997364667 hasAuthorship W1997364667A5006307308 @default.
• W1997364667 hasAuthorship W1997364667A5009092217 @default.
• W1997364667 hasAuthorship W1997364667A5010319650 @default.
• W1997364667 hasAuthorship W1997364667A5011447117 @default.
• W1997364667 hasAuthorship W1997364667A5014351060 @default.
• W1997364667 hasAuthorship W1997364667A5015688454 @default.
• W1997364667 hasAuthorship W1997364667A5017971531 @default.
• W1997364667 hasAuthorship W1997364667A5018872449 @default.
• W1997364667 hasAuthorship W1997364667A5019825165 @default.
• W1997364667 hasAuthorship W1997364667A5019831101 @default.
• W1997364667 hasAuthorship W1997364667A5020534545 @default.
• W1997364667 hasAuthorship W1997364667A5020899301 @default.
• W1997364667 hasAuthorship W1997364667A5021635558 @default.
• W1997364667 hasAuthorship W1997364667A5022042272 @default.
• W1997364667 hasAuthorship W1997364667A5022927417 @default.
• W1997364667 hasAuthorship W1997364667A5025484280 @default.
• W1997364667 hasAuthorship W1997364667A5026167700 @default.
• W1997364667 hasAuthorship W1997364667A5028306374 @default.

• next