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Page 1
Mass measurements of very neutron-deficient Mo and Tc isotopes and their impact on rp process nucleosynthesis.
Haettner E, Ackermann D, Audi G, Blaum K, Block M, Eliseev S, Fleckenstein T, Herfurth F, Hessberger FP, Hofmann S, Ketelaer J, Ketter J, Kluge HJ, Marx G, Mazzocco M, Novikov YN, Plass WR, Rahaman S, Rauscher T, Rodríguez D, Schatz H, Scheidenberger C, Schweikhard L, Sun B, Thirolf PG, Vorobjev G, Wang M, Weber C. Haettner E, et al. Among authors: schatz h. Phys Rev Lett. 2011 Mar 25;106(12):122501. doi: 10.1103/PhysRevLett.106.122501. Epub 2011 Mar 21. Phys Rev Lett. 2011. PMID: 21517310
β Decay of ^{61}V and its Role in Cooling Accreted Neutron Star Crusts.
Ong WJ, Brown EF, Browne J, Ahn S, Childers K, Crider BP, Dombos AC, Gupta SS, Hitt GW, Langer C, Lewis R, Liddick SN, Lyons S, Meisel Z, Möller P, Montes F, Naqvi F, Pereira J, Prokop C, Richman D, Schatz H, Schmidt K, Spyrou A. Ong WJ, et al. Among authors: schatz h. Phys Rev Lett. 2020 Dec 31;125(26):262701. doi: 10.1103/PhysRevLett.125.262701. Phys Rev Lett. 2020. PMID: 33449748
Mass measurement on the rp-process waiting point 72Kr.
Rodríguez D, Kolhinen VS, Audi G, Aystö J, Beck D, Blaum K, Bollen G, Herfurth F, Jokinen A, Kellerbauer A, Kluge HJ, Oinonen M, Schatz H, Sauvan E, Schwarz S. Rodríguez D, et al. Among authors: schatz h. Phys Rev Lett. 2004 Oct 15;93(16):161104. doi: 10.1103/PhysRevLett.93.161104. Epub 2004 Oct 14. Phys Rev Lett. 2004. PMID: 15524973
Production and beta decay of rp-process nuclei 96Cd, 98In, and 100Sn.
Bazin D, Montes F, Becerril A, Lorusso G, Amthor A, Baumann T, Crawford H, Estrade A, Gade A, Ginter T, Guess CJ, Hausmann M, Hitt GW, Mantica P, Matos M, Meharchand R, Minamisono K, Perdikakis G, Pereira J, Pinter J, Portillo M, Schatz H, Smith K, Stoker J, Stolz A, Zegers RG. Bazin D, et al. Among authors: schatz h. Phys Rev Lett. 2008 Dec 19;101(25):252501. doi: 10.1103/PhysRevLett.101.252501. Epub 2008 Dec 17. Phys Rev Lett. 2008. PMID: 19113700
Constraining the Neutron Star Compactness: Extraction of the ^{23}Al(p,γ) Reaction Rate for the rp Process.
Wolf C, Langer C, Montes F, Pereira J, Ong WJ, Poxon-Pearson T, Ahn S, Ayoub S, Baumann T, Bazin D, Bender PC, Brown BA, Browne J, Crawford H, Cyburt RH, Deleeuw E, Elman B, Fiebiger S, Gade A, Gastis P, Lipschutz S, Longfellow B, Meisel Z, Nunes FM, Perdikakis G, Reifarth R, Richter WA, Schatz H, Schmidt K, Schmitt J, Sullivan C, Titus R, Weisshaar D, Woods PJ, Zamora JC, Zegers RGT. Wolf C, et al. Among authors: schatz h. Phys Rev Lett. 2019 Jun 14;122(23):232701. doi: 10.1103/PhysRevLett.122.232701. Phys Rev Lett. 2019. PMID: 31298878
Exploiting Isospin Symmetry to Study the Role of Isomers in Stellar Environments.
Hallam S, Lotay G, Gade A, Doherty DT, Belarge J, Bender PC, Brown BA, Browne J, Catford WN, Elman B, Estradé A, Hall MR, Longfellow B, Lunderberg E, Montes F, Moukaddam M, O'Malley P, Ong WJ, Schatz H, Seweryniak D, Schmidt K, Timofeyuk NK, Weisshaar D, Zegers RGT. Hallam S, et al. Among authors: schatz h. Phys Rev Lett. 2021 Jan 29;126(4):042701. doi: 10.1103/PhysRevLett.126.042701. Phys Rev Lett. 2021. PMID: 33576674
Mass measurements beyond the major r-process waiting point 80Zn.
Baruah S, Audi G, Blaum K, Dworschak M, George S, Guénaut C, Hager U, Herfurth F, Herlert A, Kellerbauer A, Kluge HJ, Lunney D, Schatz H, Schweikhard L, Yazidjian C. Baruah S, et al. Among authors: schatz h. Phys Rev Lett. 2008 Dec 31;101(26):262501. doi: 10.1103/PhysRevLett.101.262501. Phys Rev Lett. 2008. PMID: 19437636
Mass measurements demonstrate a strong N=28 shell gap in argon.
Meisel Z, George S, Ahn S, Browne J, Bazin D, Brown BA, Carpino JF, Chung H, Cyburt RH, Estradé A, Famiano M, Gade A, Langer C, Matoš M, Mittig W, Montes F, Morrissey DJ, Pereira J, Schatz H, Schatz J, Scott M, Shapira D, Smith K, Stevens J, Tan W, Tarasov O, Towers S, Wimmer K, Winkelbauer JR, Yurkon J, Zegers RG. Meisel Z, et al. Among authors: schatz h, schatz j. Phys Rev Lett. 2015 Jan 16;114(2):022501. doi: 10.1103/PhysRevLett.114.022501. Epub 2015 Jan 15. Phys Rev Lett. 2015. PMID: 25635542
Mass Measurement of 56Sc Reveals a Small A = 56 Odd-Even Mass Staggering, Implying a Cooler Accreted Neutron Star Crust.
Meisel Z, George S, Ahn S, Bazin D, Brown BA, Browne J, Carpino JF, Chung H, Cole AL, Cyburt RH, Estradé A, Famiano M, Gade A, Langer C, Matoš M, Mittig W, Montes F, Morrissey DJ, Pereira J, Schatz H, Schatz J, Scott M, Shapira D, Smith K, Stevens J, Tan W, Tarasov O, Towers S, Wimmer K, Winkelbauer JR, Yurkon J, Zegers RG. Meisel Z, et al. Among authors: schatz h, schatz j. Phys Rev Lett. 2015 Oct 16;115(16):162501. doi: 10.1103/PhysRevLett.115.162501. Epub 2015 Oct 16. Phys Rev Lett. 2015. PMID: 26550869
438 results