Direct (α,p) Reaction Measurements with HELIOS and the study of 20 Ne(α,p) 23 Na
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1 Direct (α,p) Reaction Measurements with HELIOS and the study of 20 Ne(α,p) 23 Na Jianping Lai, Daniel Santiago-Gonzalez Catherine M. Deibel Louisiana State University 9/13/16 INPC
2 (α,p) Reactions in Explosive Nucleosynthesis - XRBs Type I X-ray bursts (XRBs): thermonuclear explosions on neutron star surface in binary system T peak = 1 2 GK time scale s recurrent events (hours to days) Nucleosynthesis: triple-α process CNO breakout 18 Ne(α,p) 21 Na (α,p) process rapid proton capture (rp) process synthesis up to A~100 αp-process Triple α-process rp-process H. Grawe et al., "Rep. Prog. Phys." (2007). 2
3 (α,p) Reactions in Explosive Nucleosynthesis - XRBs Sensitivity studies of XRB nucleosynthesis: vary reactions individually show only a handful of reactions significantly effect bursts Cyburt et al., 2016 (submitted) Effects of (α,p) reactions in XRBs: shape of light curve energy output elemental abundances double-peaked bursts(?) J.L. Fisker, et al., ApJ (2004). 3
4 (α,p) Reactions in Explosive Nucleosynthesis - SNeIa Type Ia Supernovae: thermonuclear explosion of white dwarf star in binary system progenitor uncertain disruptive explosion; no remnant Tpeak ~ 8 GK (α,p) Nucleosynthesis in SNeIa: C+C, C+O, O+O fusion α-chain reactions production of >50% Fe content of Galaxy Bravo et al., PRC 85, (2012) C. M. Deibel INPC September 13,
5 Type Ia Supernovae Sensitivity Studies Variation of reaction rates by factor of 10 up and down Two independent studies show high sensitivity to: 12 C(α,γ) 16 O 12 C + 12 C 20 Ne(α,p) 23 Na 20 Ne(α,γ) 24 Mg 30 Si(p,γ) 31 P >10% effects (α,p) Bravo et al., PRC 85, (2012) 5
6 Type Ia Supernovae Sensitivity Studies Variation of reaction rates by factor of 10 up and down Two independent studies show high sensitivity to: 12 C(α,γ) 16 O 12 C + 12 C 20 Ne(α,p) 23 Na 20 Ne(α,γ) 24 Mg 30 Si(p,γ) 31 P A. Parikh et al., A&A 557, 11 (2013) 6
7 Type Ia Supernovae Sensitivity Studies Variation of reaction rates by factor of 10 up and down Two independent studies show high sensitivity to: 12 C(α,γ) 16 O 12 C + 12 C 20 Ne(α,p) 23 Na 20 Ne(α,γ) 24 Mg 30 Si(p,γ) 31 P A. Parikh et al., A&A 557, 11 (2013) 7
8 Direct (α,p) measurements with HELIOS at Argonne National Laboratory 8
9 Direct (α,p) measurements with HELIOS HELIcal Orbit Spectrometer (HELIOS) repurposed MRI magnet magnetic field aligned with beam axis commissioned 2008 Ideal for studying reactions with radioactive ion beams unique particle identification from time-of-flight high geometrical efficiency improve resolution (avoid kinematic compression) Beam Prototype Si array Target fan Recoil Detector 9
10 Direct (α,p) measurements with HELIOS Direct (α,p) measurement needs: 4 He gas target cryogenically cooled commissioned with 14 C(d,p) 15 C, 14 C( 3 He,d) 15 N Spring
11 Direct (α,p) measurements with HELIOS Direct (α,p) measurement needs: 4 He gas target cryogenically cooled commissioned with 14 C(d,p) 15 C, 14 C( 3 He,d) 15 N Spring 2013 CD 2 solid target 500 mbar D 2 (gas target) 11
12 Direct (α,p) measurements with HELIOS Direct (α,p) measurement needs: 4 He gas target cryogenically cooled commissioned with 14 C(d,p) 15 C, 14 C( 3 He,d) 15 N Spring 2013 heavy-ion recoil detector recoil identification beam monitoring/normalization position information 12
13 Direct (α,p) measurements with HELIOS Direct (α,p) measurement needs: 4 He gas target cryogenically cooled commissioned with 14 C(d,p) 15 C, 14 C( 3 He,d) 15 N Spring 2013 heavy-ion recoil detector recoil identification beam monitoring/normalization position information high rate: 500 khz energy resolution: <5% position sensitivity!e (Channel) mass separation at low A 29 P 28 Si 30 S Eres (Channel) 13
14 First Direct (α,p) Study with HELIOS: 20 Ne(α,p) 23 Na Direct study of 20 Ne(α,p) 23 Na protons detected in HELIOS Si array 23 Na detected in ionization chamber normalized via known (d,p) reaction Part I completed December 2014 E beam = 107, 100, 88 MeV 23 Na NOTHING ΔE1 20 Ne 500 Torr 4 He gas ΔE1 20 Ne empty cell ΔE2 ΔE2 14
15 First Direct (α,p) Study with HELIOS: 20 Ne(α,p) 23 Na Direct study of 20 Ne(α,p) 23 Na protons detected in HELIOS Si array 23 Na detected in ionization chamber normalized via known (d,p) reaction Part I completed December 2014 E beam = 107, 100, 88 MeV 500 mbar 4 He empty gas cell Eproton (MeV) Eproton (MeV) z (cm) z (cm) 15
16 First Direct (α,p) Study with HELIOS: 20 Ne(α,p) 23 Na Part II completed July 2015 Normalization via (α,α) scattering and (d,p) on solid target Dissertation of Jianping Lai (LSU) August mbar 4 He empty gas cell 16
17 20 Ne(α,p) 23 Na Cross Sections Normalized cross section for 20 Ne(α,p) 23 Na: in agreement with Hauser- Feshbach calculations in agreement with inverse reaction cross section Future plans: determining contribution from excited states (present data) measurements at more (and lower) energies study affects on SNeIa models (p,α) measurement present data 17
18 Current Developments: ANASEN Array for Nuclear Astrophysics and Structure with Exotic Nuclei (ANASEN) p RIB recoil (via window) designed for direct (α,p) reaction studies extended, active gas target proportional counter Si detector array Nuclear Astrophysics measurements: 14N(α,p)17O (stable beam FSU) 18Ne(α,p)21Na (RIB from FSU) 37K(p,p)37K Kevin Macon, PhD Thesis (LSU) (first RIB ReA3) C. M. Deibel INPC September 13,
19 Current Developments: ANASEN p RIB recoil Array for Nuclear Astrophysics and Structure with Exotic Nuclei (ANASEN) (via window) designed for direct (α,p) reaction studies extended, active gas target proportional counter Si detector array Nuclear Astrophysics measurements: 14N(α,p)17O (stable beam FSU) 18Ne(α,p)21Na (RIB from FSU) 37K(p,p)37K Kevin Macon, PhD Thesis (LSU) (first RIB ReA3) 18Ne(α,p)21Na 14N(α,p)17O p C. M. Deibel INPC September 13, 2016 α" 19
20 Summary (α,p) reactions play a significant role in stellar explosive nucleosynthesis Direct measurements are challenging: radioactive ion beams gas targets low cross sections Multiple methods underdevelopment for direct (α,p) measurements: HELIcal Orbit Spectrometer (HELIOS) at ATLAS facility ANASEN JENSA gas-jet target with Si detector array First direct measurement of 20 Ne(α,p) 23 Na: proof-of-principle of HELIOS method important for Type Ia Supernova nucleosynthesis 20
21 THANKS! ANL Jason Clark John Greene Calem Hofman Ben Kay Richard Pardo Ernst Rehm Birger Back Akaa Ayangeakaa Melina Avila Louisiana State University Jianping Lai Jeff Blackmon Daniel Santiago-Gonzalez Kevin Macon (Postdoc Notre Dame) Amber Lauer (graduate student) Liudmyla Afanasieva (Postdoc - WashU) Florida State University Sergio Almaraz **ATLAS staff and operators** 21
22 Direct (α,p) measurements with HELIOS Direct (α,p) measurement needs: 4 He gas target cryogenically cooled commissioned with 14 C(d,p) 15 C, 14 C( 3 He,d) 15 N Spring 2013 heavy-ion recoil detector recoil identification beam monitoring/normalization position information φ Si detector φ Ionization Chamber high rate: 500 khz energy resolution: <5% position sensitivity mass separation at low A 22
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