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2000-2002 – Weizmann Institute of Science (download PDF)

last update: July 2013


2000 –2002 2 ½ years on a postdoctoral position won through an international competition at Weizmann Institute of Science WIS Rehovot, Israel, “The Edmond I. & Lillian S. Kaufman Postdoctoral Fellowship”.


I collaborated with Professor Michael Hass (lab CEO) and with Professor Michael Paul (from the Racah Institute of Physics, Hebrew University, Jerusalem) for:


  • - a)Pelletron 14MV, on multiple problems de Accelerator Mass Spectrometry:
    • o -Towards a measurement of the cross section for 3He(4He,γ)7Be with Accelerator Mass Spectroscopy (AMS),
    • o -Experimental limit to interstellar 244Pu abundance,
    • o -Be-10 measurements on Neolithic and Paleolithic flint tools from Israel,
    • o -An insight into Pu-244 abundance in interstellar matter,
    • o -Counting Ti-44 nuclei from the Ca-40(α,γ)Ti-44 reaction,
    • o -A window on nucleosynthesis through detection of short-lived radionuclides,
    • o -Flint mining in prehistory recorded by in situ-produced cosmogenic Be-10,
    • o -Magnet saturation and relativistic effects in accelerator-mass-spectrometry systems,
    • o -Upgrading of the AMS facility at the Koffler 14UD Pelletron accelerator

    Many such publications came out of this period of time (see the publication list).


  • - b)at the 3MV Van de Graaff accelerator, on 3 issues for Nuclear Astrophysics

    • o b1) astrophysical factor measurement S17(0) for the nuclear reaction 7Be(p,γ)8B responsible for the most energetic neutrinos coming from our Sun:
      • § -A new measurement of the proton capture rate on 7Be and the S17(0) factor,
      • § -Precision measurement of the 7Be(p,γ)8B cross section with an implanted 7Be target,
      • § -A new measurement of the proton capture rate on Be-7, New measurement of the proton capture rate on Be-7 and the S-17(0) factor

    • o b2) astrophysical factor measurement S34(0) for the nuclear reaction 3He(4He,γ)7Be responsible for the 7Be neutrinos, with the goal of normalizing all other previous results for this astrophysical factor:
      • § -Towards a measurement of the cross section for 3He(4He,γ)7Be with Accelerator Mass Spectroscopy (AMS),
      • § -Next steps on the cross section measurement for the fusion reaction 4He(3He,γ)7Be.

      • I did the design and the commissioning of the reaction gas-chamber, used to study the nuclear reaction 4He(3He,γ)7Be, and I established the experimental method for this measurement. In the end of my position there, I could test the chamber while running a preliminary experiment 4He(3He,γ)7Be at the 3MV accelerator.


        I learned to perform AMS (Accelerated Mass Spectrometry) measurements in Professor Michael Paul’s group, from Racah Institute of Physics from Hebrew University, Jerusalem. Here is what I did:

        - Chemical separation method of the 7Be nuclei from the implantation metal Cu (the method was a result of a collaboration with chemist Chana Feldstein from the Racah Institute of Physics, Hebrew University, Jerusalem)

        - Method to obtain standard probes for the AMS for the 7Be nuclei (method resulted from collaboration with Professor Michael Paul)

        - Data analysis for the 7Be counting through the AMS method.


    • o b3) study the nuclear reactions which may destroy 7Be si 7Li in our Sun
      • § I participated at Yale University, Connecticut, USA, to an USA-Israeli-Belgian cooperation experiment for Nuclear Astrophysics (spoke-person Professor Moshe Gai):
        • § -Destruction of Li-7 and Be-7 in astrophysical environments.

  • c) At ISOLDE, CERN, Geneva, I participated to a nuclear magnetic moment measurement (spoke-person Professor Michael Hass):
    • § Magnetic moment of Ne-17 using beta-NMR and tilted foil polarization


Activity results from this period were presented at renowned schools, such as:

  • § Erice school: the 22nd School on Radioactive beams in Nuclear and Astro Physics (2000), Sicily, Italy,
  • § Santa Tecla, Sicily, Italy : The 1st European Summer School on Astrophysics (2001),
  • § TRIUMF, Vancouver BC, Canada (2002) : SNIT 2002, Summer Nuclear Institute at TRIUMF 2002, June 10-21, 2002

and at international conferences, as:

    - AMS (see the publication list)

    § -Carbon-dating (2000) (see the publication list)

    § -Nuclear Astrophysics (see the publication list).



When I worked at WIS, for the AMS, I accomplished:

  • - Carrying out the method of AMS detection of the 7Be nuclei (and perfecting it), which allow counting the atoms created in the reaction 3He +4 He (see list of publications).
  • - I worked in chemistry labs from WIS and from the Hebrew University to determine the chemistry to be used for the preparation of 7Be probes for AMS.
  • - I participated in the completion of the computerized control of the 14MV Pelletron AMS, using LabVIEW, and to its technical implementation (see list of publications).
  • - I did relativistic calculations to calibrate the analyzing magnet from Pelletron for the case of relativistic heavy ion experiments AMS done at the time (see list of publications).


For the Nuclear Astrophysics, at WIS, I accomplished two big activities at the accelerator Van de Graaff of 3 MV:

  • - for the p+7Be experiment
    • o up-grading the existing experimental set-up
    • o Participating in the experimental group to fulfill the experiment

  • - for the 3He+4He experiment
    • o gas-target chamber construction, starting with designing and testing it
    • o the whole experimental assembly and method testing by running a preliminary experiment for the 3He+4He experiment.


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