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Nuclei in the Cosmos XV

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Cover of 'Nuclei in the Cosmos XV'

Table of Contents

  1. Altmetric Badge
    Book Overview
  2. Altmetric Badge
    Chapter 1 Resonances in Stellar Carbon Fusion
  3. Altmetric Badge
    Chapter 2 On the Mass of Supernova Progenitors: The Role of the $$^{12}$$ C $$+^{12}$$ C Reaction
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    Chapter 3 The 12 C+ 12 C Fusion Reaction at Stellar Energies
  5. Altmetric Badge
    Chapter 4 The Resonant Behaviour of the $$^{12}$$ C+ $$^{12}$$ C Fusion Cross Section at Astrophysical Energies
  6. Altmetric Badge
    Chapter 5 $$^{7}$$ Be(n,p) $$^{7}$$ Li Cross Section Measurement for the Cosmological Lithium Problem at the n $$\_$$ TOF Facility at CERN
  7. Altmetric Badge
    Chapter 6 Cross Section Measurements of the 7 Be(n,p) 7 Li and the 7 Be(n,α) 4 He Reactions Covering the Big-Bang Nucleosynthesis Energy Range by the Trojan Horse Method at CRIB
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    Chapter 7 Non-extensive Solution to Cosmological Lithium Problem
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    Chapter 8 Experimental Challenge to the Cosmological Li Problem
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    Chapter 9 The Cosmologically Relevant $$^7$$ Be(n, $$\alpha $$ ) $$^4$$ He Reaction in View of the Recent THM Investigations
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    Chapter 10 Few-Nucleon Reactions of Astrophysical Interest: A Review
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    Chapter 11 Data for the s Process from n_TOF
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    Chapter 12 The Study of the $$^{6}$$ Li(p, $$\gamma $$ ) $$^{7}$$ Be Reaction at LUNA
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    Chapter 13 A New Measurement of the $$^{2}$$ H(p, $$\gamma $$ ) $$^{3}$$ He Cross Section in the BBN Energy Range at LUNA
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    Chapter 14 Galactic Chemical Evolution with Rotating Massive Star Yields
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    Chapter 15 Inhomogeneous Chemical Evolution of r-Process Elements in the Galactic Halo
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    Chapter 16 Nucleosynthesis in Core-Collapse Supernovae
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    Chapter 17 Neutron Star Mergers as r-Process Sources
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    Chapter 18 Impact of Electron-Captures on N = 50 Nuclei on Core-Collapse Supernovae
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    Chapter 19 Learning About Nucleosynthesis from Multi-dimensional Simulations of Core-Collapse Supernovae
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    Chapter 20 Fission Properties Relevant for GW170817
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    Chapter 21 Explosive Nucleosynthesis: What We Learned and What We Still Do Not Understand
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    Chapter 22 The Beta-Oslo Method: Experimentally Constrained ( $$n,\gamma $$ ) Reaction Rates Relevant to the r -Process
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    Chapter 23 Assessment of Stellar Nucleosynthesis Abundances Using ENDF/B-VIII.0 and TENDL-2015 Evaluated Nuclear Data Libraries
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    Chapter 24 Axions and the Final Fate of Stars
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    Chapter 25 Neutrinos from Pair Instability Supernovae
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    Chapter 26 Neutrinos from Presupernova Stars
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    Chapter 27 The Chemical Composition of the Solar System
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    Chapter 28 Observational Constraints on Nucleosynthesis from AGB and Post-AGB Stars in Our Galaxy and Its Satellites
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    Chapter 29 Heavy Elements Nucleosynthesis on Accreting White Dwarfs Surface: Seeding the p-Process
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    Chapter 30 The Importance of the $$^{13}$$ C( $$\alpha $$ ,n) $$^{16}$$ O Reaction in Asymptotic Giant Branch Stars
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    Chapter 31 Thermonuclear Supernovae: Prospecting in the Age of Time-Domain and Multi-wavelength Astronomy
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    Chapter 32 Experimental Study of the $${^{30}}{\text {P}({\text {p}}}{,}{\upgamma })^{31}\text {S}$$ Reaction in Classical Novae
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    Chapter 33 s-Processing from MHD-Induced Mixing and Isotopic Abundances in Presolar SiC Grains
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    Chapter 34 The Evolution of CNO Isotope Ratios: A Litmus Test for Stellar IMF Variations in Galaxies Across Cosmic Time
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    Chapter 35 Direct $$^{13}$$ C $$(\alpha $$ ,n $$)^{16}$$ O Cross Section Measurement at Low Energies
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    Chapter 36 Nuclear AstroPhysics at ELI-NP: Preliminary Experiments with ELISSA Detector
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    Chapter 37 Direct Charged-Particle Measurements Using Stable Beams Above Ground
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    Chapter 38 Neutron Induced Reactions in Astrophysics
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    Chapter 39 Progress of Underground Nuclear Astrophysics Experiment JUNA in China
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    Chapter 40 Trojan Horse Method: A Versatile Tool for Nuclear Astrophysics
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    Chapter 41 Nuclear Reaction of Astrophysical Interest with LUNA Projects
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    Chapter 42 Investigation of neutron-induced reaction at the Goethe University Frankfurt
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    Chapter 43 Nuclear Astrophysics Underground: Status and Future
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    Chapter 44 Study on Explosive Nucleosynthesis with Low-Energy RI Beams at CRIB
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    Chapter 45 Charged-Particle Decays of Highly Excited States in $$^{19}$$ F
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    Chapter 46 Pulse Shape Discrimination for High Pressure $$^{3}$$ He Counters
  48. Altmetric Badge
    Chapter 47 Photoneutron Reaction Cross Section Measurements on 94 Mo and 90 Zr Relevant to the p -Process Nucleosynthesis
  49. Altmetric Badge
    Chapter 48 First Time Measurement of the $$^{19}$$ F(p, $$\alpha _1$$ ) $$^{16}$$ O Reaction at Astrophysical Energies: Evidence of Resonances Through the Application of the Trojan Horse Method
  50. Altmetric Badge
    Chapter 49 Aluminium-26 from Massive Binary Stars
  51. Altmetric Badge
    Chapter 50 Study of the E $$_{\alpha }$$ = 395 keV Resonance of the 22 Ne(α, γ) 26 Mg Reaction at LUNA
  52. Altmetric Badge
    Chapter 51 The s-Process Nucleosynthesis in Low Mass Stars: Impact of the Uncertainties in the Nuclear Physics Determined by Monte Carlo Variations
  53. Altmetric Badge
    Chapter 52 Stellar Nucleosynthesis: Experimental Yields of the 112 Sn(γ,n) 111 Sn and 112 Sn(γ,p) 111 m , g In Reactions for p-Nuclei Production Simulation
  54. Altmetric Badge
    Chapter 53 The Development of 400 kV High Intensity Accelerator Facility for Jinping Underground Nuclear Astrophysics Experiments
  55. Altmetric Badge
    Chapter 54 $$\mathrm {^{7}}$$ Be(p,p) $$\mathrm {^{7}}$$ Be and Its Importance in Nuclear Astrophysics
  56. Altmetric Badge
    Chapter 55 Direct Measurement of the $$^{13}C(\alpha ,n)^{16}O$$ Reaction at LUNA
  57. Altmetric Badge
    Chapter 56 H-He Shell Interactions and Nucleosynthesis in Massive Population III Stars
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    Chapter 57 A Public Code for Precision Big Bang Nucleosynthesis with Improved Helium-4 Predictions
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    Chapter 58 The LUNA Neutron Detector Array for the Direct Measurement of the $$^{13}{\hbox {C}}$$ ( $$\alpha $$ ,n) $$^{16}{\hbox {O}}$$ Nuclear Reaction
  60. Altmetric Badge
    Chapter 59 On Barium Stars and the s -Process in AGB Stars
  61. Altmetric Badge
    Chapter 60 The $$^{19}\mathrm{F}( \alpha ,\mathrm{p})^{22}$$ Ne and $$^{23}\mathrm{Na}(\mathrm{p},\alpha )^{20}$$ Ne Reactions at Energies of Astrophysical Interest via the Trojan Horse Method
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    Chapter 61 The HEAT Project: Study of Hydrogen Desorption from Carbon Targets
  63. Altmetric Badge
    Chapter 62 Explosion of Fast Spinning Sub-Chandrasekhar Mass White Dwarfs
  64. Altmetric Badge
    Chapter 63 Low-Energy Resonances and Direct Capture Cross Section in the $${^{22}}\text {Ne}(\text {p},\gamma )^{23}\text {Na}$$ Reaction
  65. Altmetric Badge
    Chapter 64 Theoretical Calculation of the p- $${}^6\text {Li}$$ Radiative Capture
  66. Altmetric Badge
    Chapter 65 Indirect $$(n, \gamma )^{91,92}$$ Zr Cross Section Measurements for the s-Process
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    Chapter 66 Heavy Puzzle Pieces: Learning About the  i Process from Pb Abundances
  68. Altmetric Badge
    Chapter 67 Women Scientists Who Made Nuclear Astrophysics
  69. Altmetric Badge
    Chapter 68 Presolar SiC Grains of Type AB with Isotopically Light Nitrogen: Contributions from Supernovae?
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    Chapter 69 Alpha-Capture Reaction Rate for $$^{22}$$ Ne( $$\alpha $$ , n) via Sub-Coulomb $$\alpha $$ -Transfer and Its Effect on Final Abundances of s-Process Isotopes
  71. Altmetric Badge
    Chapter 70 On the Activation Method for Stellar Cross-Sections Measurements: Flat Sample Correction in Measurements Relatives to Gold
  72. Altmetric Badge
    Chapter 71 Relative Importance of Convective Uncertainties
  73. Altmetric Badge
    Chapter 72 Weak Interference Between the 1 $$^-$$ States in the Vicinity of $$\alpha $$ -Particle Threshold of  $$^{16}$$ O
  74. Altmetric Badge
    Chapter 73 The Effects of $$^{26}$$ Al Isomeric State on Its Ground State Production
  75. Altmetric Badge
    Chapter 74 Spectroscopic Study on $$^{ 39 }$$ Ca Using the  $$^{ 40 }$$ Ca(d,t) $$^{ 39 }$$ Ca Reaction for Classical Nova Endpoint Nucleosynthesis
  76. Altmetric Badge
    Chapter 75 Inhomogeneous Primordial Magnetic Field Strength and Its Impact on Primordial Nucleosynthesis
  77. Altmetric Badge
    Chapter 76 Systematic Low-Energy Enhancement of the Gamma-Ray Strength Function
  78. Altmetric Badge
    Chapter 77 Impacts of the New Carbon Fusion Cross Sections on Type Ia Supernovae
  79. Altmetric Badge
    Chapter 78 A BGO Set-Up for the $$\mathbf {\mathrm {^2H(p,\varvec{\gamma })^3He}}$$ Cross Section Measurement at the BBN Energy Range
  80. Altmetric Badge
    Chapter 79 Cosmic-Ray Nucleosynthesis in Galactic Interactions
  81. Altmetric Badge
    Chapter 80 First Radiative Proton-Capture Cross-Section Measurements in Mid-Weight Nuclei Relevant to the p -Process
  82. Altmetric Badge
    Chapter 81 Radiative Alpha Capture on 7 Be with DRAGON at Energies Relevant to the $$\varvec{\nu }$$ p-Process
  83. Altmetric Badge
    Chapter 82 Uncertainties in the Production of p Nuclides in SN Ia Determined by Monte Carlo Variations
  84. Altmetric Badge
    Chapter 83 Germanium Detector Based Study of the $$^{2}$$ H(p, $$\gamma $$ ) $$^{3}$$ He Cross Section at LUNA
  85. Altmetric Badge
    Chapter 84 R-Process Nucleosynthesis in Core-Collapse Supernova Explosions and Binary Neutron Star Mergers
  86. Altmetric Badge
    Chapter 85 Precise Measurement of the $$^{95}$$ Ru and  $$^{95}$$ Tc Half-Lives
  87. Altmetric Badge
    Chapter 86 Stellar Yields of Rotating Pair Instability Supernovae and Comparison with Observations
  88. Altmetric Badge
    Chapter 87 Stellar Surface Abundance of Light Elements and Updated ( p , $$\alpha $$ ) Reaction Rates
  89. Altmetric Badge
    Chapter 88 Improving Nuclear Data Input for r-Process Calculations Around A $$\sim $$ 80
  90. Altmetric Badge
    Chapter 89 Development of an Ionization Chamber for the Measurement of the $$^{16}$$ O(n, $${\alpha }$$ ) $$^{13}$$ C Cross-Section at the CERN n_TOF Facility
  91. Altmetric Badge
    Chapter 90 The Effects of a Late Single-Star Contamination of the Solar Nebula on the Early Solar System Radioactivities
  92. Altmetric Badge
    Chapter 91 On the Measurements of the Beam Characteristics of Low-Energy Accelerator
  93. Altmetric Badge
    Chapter 92 The Nuclear Physics Uncertainty on Kilonova Heating Rates and the Role of Fission
Attention for Chapter 51: The s-Process Nucleosynthesis in Low Mass Stars: Impact of the Uncertainties in the Nuclear Physics Determined by Monte Carlo Variations
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About this Attention Score

  • In the top 25% of all research outputs scored by Altmetric
  • Good Attention Score compared to outputs of the same age (79th percentile)
  • High Attention Score compared to outputs of the same age and source (93rd percentile)

Mentioned by

1 blog
4 tweeters
1 Facebook page

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Chapter title
The s-Process Nucleosynthesis in Low Mass Stars: Impact of the Uncertainties in the Nuclear Physics Determined by Monte Carlo Variations
Chapter number 51
Book title
Nuclei in the Cosmos XV
Published in
arXiv, January 2019
DOI 10.1007/978-3-030-13876-9_51
Book ISBNs
978-3-03-013875-2, 978-3-03-013876-9

G. Cescutti, R. Hirschi, N. Nishimura, T. Rauscher, J. den Hartogh, A. St. J. Murphy, S. Cristallo, Gabriele Cescutti, Raphael Hirschi, Nobuya Nishimura, Thomas Rauscher, Jacqueline den Hartogh, Alex St. J. Murphy, Sergio Cristallo

Twitter Demographics

The data shown below were collected from the profiles of 4 tweeters who shared this research output. Click here to find out more about how the information was compiled.

Mendeley readers

The data shown below were compiled from readership statistics for 3 Mendeley readers of this research output. Click here to see the associated Mendeley record.

Geographical breakdown

Country Count As %
Unknown 3 100%

Demographic breakdown

Readers by professional status Count As %
Student > Postgraduate 1 33%
Student > Doctoral Student 1 33%
Student > Master 1 33%
Readers by discipline Count As %
Physics and Astronomy 3 100%

Attention Score in Context

This research output has an Altmetric Attention Score of 10. This is our high-level measure of the quality and quantity of online attention that it has received. This Attention Score, as well as the ranking and number of research outputs shown below, was calculated when the research output was last mentioned on 13 October 2018.
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