A. Rischka

$\text{Direct}~Q\text{-Value Determination of the}~β^-~\text{Decay of} ~^{187}\text{Re}$

P. Filianin [1], C. Lyu [1], M. Door [1], K. Blaum [1,2], W. J. Huang, M. Haverkort [3], P. Indelicato [4,1], C. H. Keitel, K. Kromer [1], D. Lange [1,5,6], Y. N. Novikov, A. Rischka [7,1], R. X. Schüssler, Ch. Schweiger [1], S. Sturm [1], S. Ulmer [8], Z. Harman [1], S. Eliseev [1]

Abstract

The cyclotron frequency ratio of $^{187}\mathrm{Os}^{29+}$ to $^{187}\mathrm{Re}^{29+}$ ions was measured with the Penning-trap mass spectrometer PENTATRAP. The achieved result of $R=1.000\:000\:013\:882(5)$ is to date the most precise such measurement performed on ions. Furthermore, the total binding-energy difference of the 29 missing electrons in Re and Os was calculated by relativistic multiconfiguration methods, yielding the value of $ΔE = 53.5(10)$ eV. Finally, using the achieved results, the mass difference between neutral $^{187}$Re and $^{187}$Os, i.e., the $Q$ value of the $β^-$ decay of $^{187}$Re, is determined to be 2470.9(13) eV.

Direct Measurement of the Mass Difference of Ho163 and Dy163 Solves the Q-Value Puzzle for the Neutrino Mass Determination

S. Eliseev [1], K. Blaum [1], M. Block [2,3,4], S. Chenmarev [1,5], H. Dorrer [4,6,7,2,3,8], Ch. E. Duellmann, C. Enss [9,1,5], P. E. Filianin, L. Gastaldo [9], M. Goncharov [1,10,2,5,11], U. Koester, F. Lautenschlaeger, Yu. N. Novikov, A. Rischka [1], R. X. Schuessler, L. Schweikhard [12,6,7], A. Tuerler

Abstract

The atomic mass difference of 163Ho and 163Dy has been directly measured with the Penning trap mass spectrometer SHIPTRAP applying the novel phase imaging ion cyclotron resonance technique. Our measurement has solved the long standing problem of large discrepancies in the Q value of the electron capture in 163Ho determined by different techniques. Our measured mass difference shifts the current Q value of 2555(16) eV evaluated in the Atomic Mass Evaluation 2012 [G. Audi et al., Chin. Phys. C 36, 1157 (2012)] by more than 7 sigma to 2833(30stat)(15sys) eV/c2. With the new mass difference it will be possible, e.g., to reach in the first phase of the ECHo experiment a statistical sensitivity to the neutrino mass below 10 eV, which will reduce its present upper limit by more than an order of magnitude.