Vegetation of the Peak District / C. E. Moss.

Abstract

Address by Congressman John E. Moss JOt-IN E. MOSS: For over twenty years, Congressman Moss has represented the Third Congressional District of California. He serves on the lnterstate and Foreign Comnierce Committee and the Government Operations Committee as velI as on several subcommittees He is chairman of the Subcommittee on Commerce and Finance of the Committee on Interstate and Foreign Commerce, which has legislative responsibility for securities matters in the House of Representatives. Mr. Moss also is chairman of the Foreign Operations and Government Information Subcommittee ot the Government Operations Committee.

One-neutron knockout reactions on proton-rich nuclei withN=16

“…The neutron single-particle structure of 31 S has been studied extensively with ͑p , d͒ [34,35], ͑d , t͒ [36][37][38], and ͑ 3 He, ␣͒ [39,40] transfer reactions at low energies (see Refs. [41,42] for the evaluated summaries).…”

NewP30(p,γ)Wrede1, Caggiano2, Clark3 et al. 2007Phys. Rev. C351342View full textAdd to dashboardCite

“…The 223.8 (25) keV ( = 2) resonance now makes only a minor 2-11% contribution to the rate for 0.10 < T < 0.30 GK.…”

“…All known 31 S states from the proton threshold to 6.7 MeV were populated, three previously unresolved resonances were excited, and the existence of a 6585(2) keV level observed to date only tentatively was confirmed [25]. 1 Where excitation energy uncertainties are not quoted directly in Ref.…”

“…remains dominant for 0.02 < T < 0.08 GK and the 410.1 (25) and 452.1 (25) keV resonances still dominate for 0.25 < T < 0.4 GK. The 223.8 (25) keV ( = 2) resonance now makes only a minor 2-11% contribution to the rate for 0.10 < T < 0.30 GK.…”

Experimental evidence for a natural parity state inMg26and its impact on the production of neutrons for thesprocess

“…The 22 Ne(α, n) 25 Mg reaction is regarded as the main neutron source for the s process in core He-burning massive stars [1] and is of relevance in He-shell burning in AGB stars [2]. Our current understanding of its rate is one of the most important sources of uncertainty in the nucleosynthesis of heavy elements.…”