The masses of six neutron-deficient rare holmium and thulium isotopes close to the proton drip line were determined with the SHIPTRAP Penning trap mass spectrometer. For the first time the masses of the proton-unbound isotopes 144,145Ho and 147,148Tm were directly measured. The proton separation energies were derived from the measured mass values and compared to predictions from mass formulas. The new values of the proton separation energies are used to determine the location of the proton drip line for holmium and thulium more accurately.
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http://dx.doi.org/10.1103/PhysRevLett.100.012501 | DOI Listing |
Postgrad Med
November 2024
Division of Critical Care Medicine, St Mary's General Hospital, Passaic, NJ, USA.
Acta Gastroenterol Belg
August 2024
The Gonczarowski Family Institute of Gastroenterology and Liver Diseases, Shamir (Assaf Harofeh) Medical Center, Zerifin, Israel and The Faculty of Medicine, Tel Aviv University, Tel Aviv, Israel.
Phys Rev Lett
June 2024
Department of Physics, Technische Universität Darmstadt, D-64289 Darmstadt, Germany.
Neutron stars contain neutron-rich matter with around 5% protons at nuclear saturation density. In this Letter, we consider equilibrium between bulk phases of matter based on asymmetric nuclear matter calculations using chiral effective field theory interactions rather than, as has been done in the past, by interpolation between the properties of symmetric nuclear matter and pure neutron matter. Neutron drip (coexistence of nuclear matter with pure neutrons) is well established, but from earlier work it is unclear whether proton drip (equilibrium between two phases, both of which contain protons and neutrons) is possible.
View Article and Find Full Text PDFPhys Rev Lett
February 2024
Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou 730000, China.
Using the fusion-evaporation reaction ^{106}Cd(^{58}Ni,4n)^{160}Os and the gas-filled recoil separator SHANS, two new isotopes _{76}^{160}Os and _{74}^{156}W have been identified. The α decay of ^{160}Os, measured with an α-particle energy of 7080(26) keV and a half-life of 201_{-37}^{+58} μs, is assigned to originate from the ground state. The daughter nucleus ^{156}W is a β^{+} emitter with a half-life of 291_{-61}^{+86} ms.
View Article and Find Full Text PDFJ Rhinol
November 2023
Department of Otorhinolaryngology-Head and Neck Surgery, Chungbuk National University College of Medicine, Chungbuk National University Hospital, Cheongju, Republic of Korea.
Background And Objectives: Laryngopharyngeal reflux (LPR) is an increasingly common disease, characterized by stomach acid reflux reaching the upper airways. Postnasal drip (PND) is a known consequence of LPR, defined as mucus accumulation perceived in the posterior areas of the nose and throat. PND is among the most common causes of persistent cough, hoarseness, sore throat, and other symptoms, affecting the quality of life.
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