Publications by authors named "E K Akhmedov"

Aim: to assess risk of development of diabetes mellitus (DM) and detection of other metabolic derangements among physicians-internists.

Material And Methods: In an open clinical screening study participated 117 male and 167 female physicians mostly cardiologists and internists from various regions of Russia. All participants filled in standard questionnaires and were subjected to examination which included measurement of height, body mass, waist circumference, determination of adipose tissue mass adiposity analyzer, registration of arterial pressure, and assessment of DM risk using Finnish Diabetes Risk Score (FINDRISC).

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We consider type I + II seesaw mechanism, where the exchanges of both right-handed neutrinos and isotriplet Higgs bosons contribute to the neutrino mass. Working in the left-right symmetric framework and assuming the mass matrix of light neutrinos m(v) and the Dirac-type Yukawa couplings to be known, we find the triplet Yukawa coupling matrix f, which carries the information about the masses and mixing of the right-handed neutrinos. We show that in this case there exists a duality: for any solution f, there is a dual solution [symbol: see text] = m(v)/nu(L) - f, where nu(L) is the vacuum expectation value of the triplet Higgs boson.

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We present a formalism for precise description of oscillation phenomena in matter at high energies or high densities, V > Delta m(2)/2E, where V is the matter-induced potential of neutrinos. The accuracy of the approximation is determined by the quantity, where is the mixing angle in matter and is a typical change of the potential over the oscillation length (). We derive simple and physically transparent formulas for the oscillation probabilities, which are valid for arbitrary matter density profiles.

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Article Synopsis
  • The study focuses on three types of light neutrinos with different mass levels, indicating that solar neutrino data can provide insights into a specific mixing element (U(e3)) of the lepton mixing matrix.
  • It suggests that if U(e3) is measured in atmospheric or long baseline experiments, it could help clarify the different theories surrounding the solar neutrino anomaly.
  • The interaction between solar neutrino data and U(e3) measurements could refine our understanding of neutrino behavior and their oscillation patterns.
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