Publications by authors named "A Pullia"

Article Synopsis
  • A search for dark matter candidates in the mass range of 65 to 1021 keV was conducted using data from the GERDA experiment, focusing on energy depositions without detecting any significant signals above background noise.
  • The study established stringent exclusion limits on dark photon and axion-like particle interactions with electrons, with specific constraints noted at a 150 keV mass level.
  • Additional investigations into the decay rates of nucleons and electrons yielded lower lifetime limits for neutron, proton, and electron decay events at a 90% confidence interval.
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The excited states of unstable ^{20}O were investigated via γ-ray spectroscopy following the ^{19}O(d,p)^{20}O reaction at 8  AMeV. By exploiting the Doppler shift attenuation method, the lifetimes of the 2_{2}^{+} and 3_{1}^{+} states were firmly established. From the γ-ray branching and E2/M1 mixing ratios for transitions deexciting the 2_{2}^{+} and 3_{1}^{+} states, the B(E2) and B(M1) were determined.

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We present the measurement of the two-neutrino double-β decay rate of ^{76}Ge performed with the GERDA Phase II experiment. With a subset of the entire GERDA exposure, 11.8 kg yr, the half-life of the process has been determined: T_{1/2}^{2ν}=(2.

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We search for tri-nucleon decays of Ge in the dataset from the GERmanium Detector Array (GERDA) experiment. Decays that populate excited levels of the daughter nucleus above the threshold for particle emission lead to disintegration and are not considered. The ppp-, ppn-, and pnn-decays lead to Cu, Zn, and Ga nuclei, respectively.

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Classical novae are thermonuclear explosions in stellar binary systems, and important sources of Al and Na. While γ rays from the decay of the former radioisotope have been observed throughout the Galaxy, Na remains untraceable. Its half-life (2.

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