- Home
- Search Results
- Page 1 of 1
Search for: All records
-
Total Resources3
- Resource Type
-
0000000003000000
- More
- Availability
-
21
- Author / Contributor
- Filter by Author / Creator
-
-
Tarasov, O_B (3)
-
Baumann, T. (2)
-
Bazin, D. (2)
-
Fukuda, N. (2)
-
Ginter, T. (2)
-
Klankowski, L. (2)
-
Liddick, S. (2)
-
Rogers, A_M (2)
-
Suzuki, H. (2)
-
Ahn, D_S (1)
-
Barber, M. (1)
-
Bender, P_C (1)
-
Bhatt, K. (1)
-
Chapman, T. (1)
-
Chen, J. (1)
-
Chowdhury, P. (1)
-
Dopfer, J. (1)
-
Estrade, A. (1)
-
Estradé, A. (1)
-
Famiano, B. (1)
-
- Filter by Editor
-
-
& Spizer, S. M. (0)
-
& . Spizer, S. (0)
-
& Ahn, J. (0)
-
& Bateiha, S. (0)
-
& Bosch, N. (0)
-
& Brennan K. (0)
-
& Brennan, K. (0)
-
& Chen, B. (0)
-
& Chen, Bodong (0)
-
& Drown, S. (0)
-
& Ferretti, F. (0)
-
& Higgins, A. (0)
-
& J. Peters (0)
-
& Kali, Y. (0)
-
& Ruiz-Arias, P.M. (0)
-
& S. Spitzer (0)
-
& Sahin. I. (0)
-
& Spitzer, S. (0)
-
& Spitzer, S.M. (0)
-
(submitted - in Review for IEEE ICASSP-2024) (0)
-
-
Have feedback or suggestions for a way to improve these results?
!
Note: When clicking on a Digital Object Identifier (DOI) number, you will be taken to an external site maintained by the publisher.
Some full text articles may not yet be available without a charge during the embargo (administrative interval).
What is a DOI Number?
Some links on this page may take you to non-federal websites. Their policies may differ from this site.
-
Abstract We measured the production cross sections and momentum distributions of proton-rich radioactive isotopes (RIs) whose atomic numbers were 18–37. These isotopes were produced by the projectile fragmentation of a 345-MeV/nucleon $$^{78}$$Kr beam impinged on a 5-mm Be target. The cross sections close to the stability region were reproduced fairly well by the semi-empirical formulas, EPAX3.1a and FRACS1.1. However, these formulas tend to overestimate the cross sections of the RIs near the proton drip line, sometimes by as much as 100-fold. The Abrasion–Ablation model in the LISE$$^{++}$$ package was employed, using different mass table variations, to describe the experimental results in this region. The best agreement was achieved when the Weizsäcker-Skyrme microscopic-macroscopic mass formula (WS4$$_{\mathrm{RBF}}$$) and a version of the nonrelativistic Hartree–Fock–Bogoliubov mass model (HFB22) were used. The momentum distribution was represented well by an asymmetric Gaussian distribution. The width of the high-momentum side of the distribution was reproduced fairly well by the Goldhaber model, whereas the width of the low-momentum side was 1.1 times larger than that of the high-momentum side. Moreover, an exponential-shaped low-momentum tail was observed, which began from a height of approximately 1/100–1/1000 of the momentum peak. The momentum means were not reproduced well by Morrissey’s empirical formula: additional velocity loss to the formula was observed. The yield of $$^{68}$$Br was smaller than the expected yield, as estimated from the yield systematics of its neighboring RIs. Assuming an in-flight decay in the separator, the half-life of $$^{68}$$Br was estimated to be $$105^{+62}_{-25}$$ ns.more » « less
-
Sharma, K.; Chowdhury, P.; Rogers, A_M; Tarasov, O_B; Haak, K.; Hoff, D_E_M; Bender, P_C; Baumann, T.; Bazin, D.; Chen, J.; et al (, Physical Review C)
-
Wang, K-L; Estrade, A.; Famiano, M.; Schatz, H.; Barber, M.; Baumann, T.; Bazin, D.; Bhatt, K.; Chapman, T.; Dopfer, J.; et al (, Physical Review C)
An official website of the United States government
