Difference between revisions of "References and Documents"

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* ''Nuclear reactions in stellar helium burning and later hydrostatic burning stages''
 
* ''Nuclear reactions in stellar helium burning and later hydrostatic burning stages''
L.R. Buchmann, C.A. Barnes, Nuclear Physics A '''777''' (2006) 254 [[media:NuclPhysA.777.254.pdf]]
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L.R. Buchmann, C.A. Barnes, Nucl. Phys. A '''777''' (2006) 254 [[media:NuclPhysA.777.254.pdf]]
 +
 
 +
* ''E1 and E2 capture cross section and astrophysical reaction rate of the key reaction <sup>12</sup>C(α,γ)<sup>16</sup>O''
 +
J.W. Hammer et. al., Nucl. Phys. A '''758''' (2005) 363 [[media:NuclPhysA.758.363.pdf]]
  
 
* ''<sup>12</sup>C(α, γ )<sup>16</sup>O: The Key Reaction in Stellar Nucleosynthesis''
 
* ''<sup>12</sup>C(α, γ )<sup>16</sup>O: The Key Reaction in Stellar Nucleosynthesis''
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* ''The E1 and E2 capture amplitudes in <sup>12</sup>C(α,γ0)<sup>16</sup>O''
 
* ''The E1 and E2 capture amplitudes in <sup>12</sup>C(α,γ0)<sup>16</sup>O''
 
G. Roters et al., Eur. Phys. J. A '''6''' (1999) 451 [[media:EurPhysJA.6.451.pdf]]
 
G. Roters et al., Eur. Phys. J. A '''6''' (1999) 451 [[media:EurPhysJA.6.451.pdf]]
 
  
 
= Nucleosynthesis =
 
= Nucleosynthesis =

Revision as of 10:47, 23 December 2013

Program Advisory Committee (PAC)


Proceedings

  • Determination of astrophysical thermonuclear rates with a bubble chamber: 12C(α,γ)16O reaction case

PEB Proceedings, [1]. AIP Conf. Proc. 1563, 239 (2013), media:AIP.1.4829419.pdf [2]


Bubble Chamber

  • First determination of an astrophysical cross section with a bubble chamber: The 15N(α,γ) 19F reaction

C. Ugalde et al., Phys. Lett. B 719 (2013) 74 media:PhysLettB.719.74.pdf

  • New insights into particle detection with superheated liquids

S. Archambault et al., New J. Phys. 13 (2011) 043006 media:NewJPhys.13.043006.pdf

  • Discrimination of nuclear recoils from alpha particles with superheated liquids

F. Aubin et al., New J. Phys. 10 (2008) 103017 media:NewJPhys.10.103017.pdf

  • Direct measurement of the bubble-nucleation energy threshold in a CF3I bubble chamber

E. Behnke et al., Phys. Rev. D 88 (2013) 021101(R) media:PhysRevD.88.021101.pdf

  • Study of low frequency acoustic signals from superheated droplet detector

P.K. Mondal et al., Nucl. Inst. Meth. A 729 (2013) 182 media:NuclInstMethA.729.182.pdf

  • Development of bubble chambers with enhanced stability and sensitivity to low-energy nuclear recoils

W.J. Bolte et al., Nucl. Inst. Meth. A 577 (2007) 569 media:NuclInstMethA.577.569.pdf

  • Response of superheated droplet detectors of the PICASSO dark matter search experiment

M. Barnabé-Heider et al., Nucl. Inst. Meth. A 555 (2005) 184 media:NuclInstMethA.555.184.pdf

  • Superheated liquid and its place in radiation physics

S.C. Roy, Radiation Physics and Chemistry 61 (2001) 271 media:RadiatPhysChem.61.271.pdf

  • Search for dark matter with moderately superheated liquids

V. Zacek, Nuovo Cimento A 107 (1994) 1247 media:NuovoCementoA.107.1247.pdf

  • On the Theory of the Bubble Chamber

F. Seitz, Phys. of Fluids 1 (1957) 2 media:Phys.Fluids.1.2.pdf


Oxygen S-Factor

  • The astrophysical S factor of 12C(α, γ )16O at stellar energy

D. Schürmann, L. Gialanella, R. Kunz, F. Strieder, Phys. Lett. B 711 (2012) 35 media:PhysLettB.711.35.pdf

  • New Determination of the Astrophysical S Factor SE1 of the 12C(α,γ)16O Reaction

X. D. Tang et al., Phys. Rev. Lett. 99 (2007) 052502 media:PhysRevLett.99.052502.pdf

  • A new study for 16O(γ,α)12C at the energies of nuclear astrophysics interest: The inverse of key nucleosynthesis reaction 12C(α,γ)16O

Y. Xu et al., Nucl. Inst. Meth. A 581 (2007) 866 media:NuclInstMethA.581.866.pdf

  • Measurement of the Cascade Transition via the First Excited State of 16O in the 12C(α,γ)16O Reaction, and Its S Factor in Stellar Helium Burning

C. Matei et al., Phys. Rev. Lett. 97 (2006) 242503 media:PhysRevLett.97.242503.pdf

  • Nuclear reactions in stellar helium burning and later hydrostatic burning stages

L.R. Buchmann, C.A. Barnes, Nucl. Phys. A 777 (2006) 254 media:NuclPhysA.777.254.pdf

  • E1 and E2 capture cross section and astrophysical reaction rate of the key reaction 12C(α,γ)16O

J.W. Hammer et. al., Nucl. Phys. A 758 (2005) 363 media:NuclPhysA.758.363.pdf

  • 12C(α, γ )16O: The Key Reaction in Stellar Nucleosynthesis

R. Kunz et al., Phys. Rev. Lett. 86 (2001) 3244 media:PhysRevLett.86.3244.pdf

  • The E1 and E2 capture amplitudes in 12C(α,γ0)16O

G. Roters et al., Eur. Phys. J. A 6 (1999) 451 media:EurPhysJA.6.451.pdf

Nucleosynthesis

  • Nucleosynthesis and remnants in massive stars of solar metallicity

S.E. Woosley and A. Heger, Phys. Reports 442 (2007) 269 media:Phys.Reports.442.269.pdf

  • Coulomb dissociation as a source of information on radiative capture processes of astrophysical interest

G. Baur et al., Nucl. Phys. A 458 (1986) 188 media:NuclPhysA.458.188.pdf

  • General properties of astrophysical reaction rates in explosive nucleosynthesis

T. Rauscher, J. Phys. Conf. Ser. 420 (2013) 012138 media:J.Phys.Conf.Ser._420_1_012138.pdf


Astrophysics

  • Dependence of s-process nucleosynthesis in massive stars on triple-alpha and 12C(α,γ)16O reaction rate uncertainties

C. Tur et al., Astroph. J., 702(2) (2009) 1068 media:AstrophJ_702_2_1068.pdf