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Black Hole

Lensing of space time around a black hole. At Oxford we study black holes observationally and theoretically on all size and time scales - it is some of our core work.

Credit: ALAIN RIAZUELO, IAP/UPMC/CNRS. CLICK HERE TO VIEW MORE IMAGES.

Jirina Stone

Visitor

Sub department

  • Astrophysics
jirina.stone@physics.ox.ac.uk
Telephone: 01865 (2)73306
Denys Wilkinson Building, room 704
  • About
  • Publications

First nuclear moment measurement with radioactive beams by recoil-in-vacuum method: g-factor of the 2(1)(+) state in Te-132

EUR PHYS J A 25 (2005) 205-208

Authors:

NJ Stone, AE Stuchbery, M Danchev, J Pavan, CL Timlin, C Baktash, C Barton, JR Beene, N Benczer-Koller, CR Bingham, J Dupak, A Galindo-Uribarri, CJ Gross, G Kumbartzki, DC Radford, JR Stone, NV Zamfir

Abstract:

Following Coulomb excitation of the radioactive ion beam (RIB) Te-132 at HRIBF, we report the first use of the recoil-in-vacuum (RIV) method to determine the g-factor of the 2(1)(+) state to be (+)0.35(5). The advantages offered by the RIV method in the context of RIBs and modern detector arrays are discussed.
More details from the publisher

Further search for the decay K+→π+νν¯ in the momentum region P<195 MeV/c

Physical Review D American Physical Society (APS) 70:3 (2004) 037102

Authors:

S Adler, M Aoki, M Ardebili, MS Atiya, AO Bazarko, PC Bergbusch, B Bhuyan, EW Blackmore, DA Bryman, I-H Chiang, MR Convery, MV Diwan, JS Frank, JS Haggerty, T Inagaki, MM Ito, V Jain, DE Jaffe, S Kabe, M Kazumori, SH Kettell, P Kitching, M Kobayashi, TK Komatsubara, A Konaka, Y Kuno, M Kuriki, TF Kycia, KK Li, LS Littenberg, JA Macdonald, RA McPherson, PD Meyers, J Mildenberger, N Muramatsu, T Nakano, C Ng, S Ng, T Numao, A Otomo, J-M Poutissou, R Poutissou, G Redlinger, T Sasaki, T Sato, T Shinkawa, FC Shoemaker, AJS Smith, R Soluk, JR Stone, RC Strand, S Sugimoto, C Witzig, Y Yoshimura
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Giant resonances from TDHF

International Journal of Modern Physics E 13:1 (2004) 181-185

Authors:

PD Stevenson, MR Strayer, J Rikovska Stone, WG Newton

Abstract:

A method of calculating giant resonance strength functions using Time-Dependent Hartree-Fock techniques is described. An application to isoscalar giant monopole resonances in spherical nuclei is made, thus allowing a comparison between independent 1-, 2- and 3-Dimensional computer codes.
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Probing the sustainability of the N=82 and Z=50 shell closures for neutron-rich nuclides: Decay of120Rh75 to levels of 120Pd74

Physical Review C - Nuclear Physics 70:3 (2004) 0343141-0343145

Authors:

WB Walters, BE Tomlin, PF Mantica, BA Brown, J Rikovska Stone, AD Davies, A Estrade, PT Hosmer, N Hoteling, SN Liddick, TJ Mertzimekis, F Montes, AC Morton, WF Mueller, M Ouellette, E Pellegrini, P Santi, D Seweryniak, H Schatz, J Shergur, A Stolz

Abstract:

The low-energy levels of 120Pd74 were populated by β decay of 120Rh75, which was produced via projectile fragmentation of a 136Xe82 beam at 120 MeV/nucleon. Delayed β-gated γ rays with energies of 438 and 618 keV were observed in coincidence with 120Rh75 fragments and assigned to the 21+ → 0+ and 41+ → 21+ transitions, respectively, in 120Pd74. Isomeric γ-ray transitions are also reported for 120Rh75 and 126Cd78. The low-energy structure of 120Pd74 shows remarkable similarity to those of the isotopic 108Pd62 and isotonic 128Xe74 suggesting that these nuclides share the same Z=50 and N=82 closed shell structures with neutron-rich 120Pd 74.
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Nuclear matter and neutron-star properties calculated with the Skyrme interaction

Physical Review C American Physical Society (APS) 68:3 (2003) 034324

Authors:

J Rikovska Stone, JC Miller, R Koncewicz, PD Stevenson, MR Strayer
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