High spin states in the two nuclei $^{52}\mathrm{Cr}$ and $^{52}\mathrm{Mn}$, with ${J}^{\ensuremath{\pi}}$\ensuremath{\le}${11}^{+}$, have been studied via the reactions $^{51}\mathrm{V}$(\ensuremath{\alpha},p2n\ensuremath{\gamma}) and $^{51}\mathrm{V}$(\ensuremath{\alpha},3n\ensuremath{\gamma}), respectively, by in-beam \ensuremath{\gamma}-ray spectroscopy. Measurements of lifetimes of excited states by the Doppler shift attenuation and recoil distance techniques, \ensuremath{\gamma}-ray angular distributions, excitation functions, and \ensuremath{\gamma}\ensuremath{\gamma} coincidence, have been carried out in both the nuclei. New results obtained in $^{52}\mathrm{Cr}$ are the mean lifetime values of ${0.35}_{\mathrm{\ensuremath{-}}0.13}^{+0.25}$, ${0.23}_{\mathrm{\ensuremath{-}}0.11}^{+0.22}$, and <2.0 ps for the three highest observed states 8216.0 (${11}^{+}$), 7237.1 (${10}^{+}$), and 6453.4 keV (${9}^{+}$), and multipole mixing ratios ${\mathrm{\ensuremath{-}}0.10}_{\mathrm{\ensuremath{-}}0.05}^{+0.08}$, ${0.06}_{\mathrm{\ensuremath{-}}0.03}^{+0.05}$, and ${\mathrm{\ensuremath{-}}0.22}_{\mathrm{\ensuremath{-}}0.15}^{+0.08}$ for the 978.9, 784.7, and 629.1 keV \ensuremath{\gamma} rays depopulating these states, respectively. In $^{52}\mathrm{Mn}$, the lifetime of the 4163.4 keV (${10}^{+}$) state, hitherto unreported, has been measured to be ${0.20}_{\mathrm{\ensuremath{-}}0.16}^{+0.35}$ ps.Lifetimes of two other states in $^{52}\mathrm{Mn}$, at 870.1 (${7}^{+}$) and 2907.9 keV (${9}^{+}$), for which only the upper limits were known previously, have been measured in this work and are found to be ${0.07}_{\mathrm{\ensuremath{-}}0.04}^{+0.08}$ and 0.12\ifmmode\pm\else\textpm\fi{}0.08 ps, respectively. A comparison of the present experimental results on level lifetimes, multipole mixing ratios, and transition probabilities with the available theoretical calculations shows that most of the levels in $^{52}\mathrm{Cr}$ with excitation energies greater than 3.4 MeV are almost pure 1p5h states, while the lower lying states have a predominantly 0p4h configuration, with \ensuremath{\sim}20% 1p5h admixture. The observed M1 and E2 transition strengths between the high spin states in $^{52}\mathrm{Mn}$ favor interpretation of these states as having predominantly (${f}_{7/2}$${)}^{n}$ configuration and provide evidence for the existence of collective features in this nucleus.
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