The 2nd International Conference on Nuclear Physics in Astrophysics (eBook)
XVI, 349 Seiten
Springer Berlin (Verlag)
978-3-540-32843-8 (ISBN)
Launched in 2004, 'Nuclear Physics in Astrophysics' has established itself in a successful topical conference series addressing the forefront of research in the field. This volume contains the selected and refereed papers of the 2nd conference, held in Debrecen in 2005 and reprinted from 'The European Physical Journal A - Hadrons and Nuclei'.
The European Physical Journal A 5
List of participants 8
Foreword 13
1 Big-Bang Nucleosynthesis 15
Big bang nucleosynthesis in the new cosmology 16
1 Introduction 16
2 Big bang nucleosynthesis theory 17
3 From nuclear data to primordial abundance predictions 19
4 Light element observations and comparison with theory 21
5 Beyond the Standard Model 23
6 Summary 25
References 25
2 Neutrino Physics 27
Salty neutrinos from the Sun 28
1 Introduction 28
2 The Sudbury Neutrino Observatory 28
3 Data analysis 30
4 Results 32
5 Conclusions 34
6 Outlook 34
References 34
Prospects in double beta decay searches 35
1 Introduction 35
2 Dirac neutrinos and Majorana neutrinos 35
3 Double beta decay 36
4 Prediction on the Majorana mass 38
5 Experimental techniques 39
6 First-generation experiments 40
7 Towards second-generation experiments 41
8 Future experiments 42
9 Conclusions 43
References 44
Search for rare processes with DAMA/LXe experiment at Gran Sasso 45
1 Introduction on previous results 45
2 The search for nucleon instabilities into invisible channels in the 136Xe isotope 46
3 Conclusion 50
References 50
On the importance of low-energy beta beams for supernova neutrino physics 52
1 Introduction 52
2 Synthetic spectra 53
3 Detector response 55
References 57
Neutrino-nucleon scattering rates in protoneutron stars and nuclear correlations in the spin S = 1 channel 58
1 Introduction 58
2 Neutrino-nucleon scattering rates 58
3 The effective nuclear interaction in the spin channel 59
4 Density dependence of the Landau parameters 60
5 Response functions 61
6 Mean free path 62
7 Conclusion and outlook 63
References 63
From DAMA/NaI to DAMA/LIBRA at LNGS 65
1 Introduction 65
2 The model-independent result of DAMA/NaI 66
3 Some corollary model-dependent quests for a candidate 67
4 Towards the future: from DAMA/NaI to DAMA/LIBRA and beyond 69
5 Conclusion 70
References 70
Searching for Majorana neutrinos with double beta decay and with beta beams 71
1 Introduction 71
2 The neutrinoless double beta processes 71
3 Searching for Majorana neutrinos with beta 3 Searching for Majorana neutrinos with beta 73
4 Helicity admixture estimates 73
5 Conclusions and outlook 74
References 74
Interactions of the solar neutrinos with the deuterons 75
1 Introduction 75
2 Weak axial nuclear exchange currents 77
3 Numerical results 77
4 Conclusions 80
References 80
3 Non-explosive Nucleosynthesis 81
Relation between the 16O(a, .)20Ne reaction and its reverse20Ne(.,a)16O reaction in stars and in the laboratory 82
1 Introduction 82
2 Resonant reaction rates 83
3 Discussion 84
4 Experiments with quasi-thermal photon spectra 84
5 Conclusions 85
References 85
Enhanced d(d,p)t fusion reaction in metals 86
1 Introduction 86
2 Setup and experimental procedure 87
3 Temperature dependence of Pt and Co 87
4 Temperature dependence of metals with high solubility at T = 20 C 88
5 Discussion 89
References 89
Experimental and theoretical screening energies for the 2H(d, p)3H reaction in metallic environments 90
1 Introduction 90
2 Experimental screening energy 90
3 Theoretical description of the electron screening effect 91
4 Comparison with results of other authors 93
5 Discussion and conclusions 94
References 94
Influence of chaos on the fusion enhancement by electron screening 96
1 Introduction 96
2 Formalism 97
3 Application to the electron screening problem 98
4 Summary 101
References 101
4 Explosive Nucleosynthesis 102
Recent astrophysical studies with exotic beams at ORNL 103
1 Introduction 103
2 Experimental details 103
3 Studies with 18F beams 104
4 Studies with 7Be beams 107
5 Studies with neutron-rich beams 108
6 Conclusions 111
References 112
Beacons in the sky: Classical novae vs. X-ray bursts 113
1 Introduction 113
2 Classical nova explosions 114
3 X-ray bursts 118
4 Outlook 119
References 120
Re-evaluating reaction rates relevant to nova nucleosynthesis from a nuclear structure perspective 122
1 Introduction 122
2 Example 1: 22Na(p, .) 123
3 Example 2: 30P(p, .) 124
4 Conclusions 125
References 126
Evidence for p-process nucleosynthesis recorded at the Solar System abundances 127
1 Introduction 127
2 Analyzing the solar abundances and discovery of the first scaling 128
3 Discovery of the second scaling 129
4 Proposal of a novel concept of the universality of the p-process 129
5 Proposal of a novel concept of rate meter for the s-process 129
6 Supernova model calculations 130
7 Proposal of a new nuclear cosmochronometer 131
8 Conclusion 132
References 132
(n, .) cross-sections of light p nuclei 133
1 Introduction 133
2 Experimental procedure 134
3 Data analysis 134
4 Results and discussion 135
5 Summary 137
6 KADoNiS —The Karlsruhe Astrophysical Database of Nucleosynthesis in Stars 138
References 138
Photodissociation of p-process nuclei studied by bremsstrahlunginduced activation 139
1 Introduction 139
2 Experimental setup 139
3 Photo-activation measurements 140
4 Conclusion 144
References 144
106,108Cd(p, .)107,109In cross-sections for the astrophysicalp-process 145
1 Introduction 145
2 Investigated reactions 146
3 Experimental procedure 146
4 Results and conclusion 148
References 148
A study of alpha capture cross-sections of 112Sn 149
1 Introduction 149
2 Experimental technique 150
3 Experimental results 151
References 152
Photodissociation of neutron de.cient nuclei 153
1 Introduction 153
2 The A ˜ 100 mass region 153
3 Coulomb dissociation experiments 154
4 Summary and outlook 155
References 156
Photonuclear reaction data and .-ray sources for astrophysics 157
1 Introduction 157
2 Direct determination of (.,n) cross sections 158
3 Perspectives 160
References 162
5 Cross-Section Measurements and Nuclear Data for Astrophysics 163
CNO hydrogen burning studied deep underground 164
1 Introduction 164
2 Which nuclear energy range is of astrophysical interest? 165
3 The 14N(p, .)15O reaction 166
4 Laboratory for Underground Nuclear Astrophysics (LUNA) 168
5 LUNA 14N(p, .)15O gas target experiment 168
6 Astrophysical scenarios that can be better understood using data from the present experiment 172
References 173
Pygmy dipole strength close to particle-separation energies —The case of the Mo isotopes 174
1 Dipole strength in heavy nuclei 174
2 Nuclear resonance .uorescence 175
3 Photon scattering experiments on Mo isotopes 176
4Dipole strength in isolated narrow resonances 176
5 Level densities and fluctuating cross sections 177
6 The distribution of photon strength and pygmy resonances 178
7 Conclusion 178
References 179
Towards a high-precision measurement of the 3He(a, .)7Be cross section at LUNA 180
1 Introduction 180
2 Experimental setup 181
3 The on-line . detection technique 182
4 The activation technique 182
References 183
Radiative and non-radiative electron capture from carbon atoms by relativistic helium ions 184
1 Introduction 184
2 Experiment 185
3 Results and discussion 186
4 Radiative electron capture by fast projectiles vs. the adiabaticity parameter 187
5 Summary and conclusions 187
References 188
Evidence for a host-material dependence of the n/p branching ratio of low-energy d+d reactions within metallic environments 189
1 Introduction 189
2 Experimental results 189
3 Theoretical considerations and discussion 193
4 Conclusion 194
References 194
New measurement of 7Be half-life in di.erent metallic environments 195
1 Introduction 195
2 Experimental procedure 196
3 Results 197
References 198
Study of the 106Cd(a, a)106Cd scattering at energies relevant to the p-process 199
1 Introduction 199
2 Experimental setup and procedure 200
3 Optical potential parameters 201
References 202
Study of fission fragments produced by 14N + 235U reaction 203
1 Introduction 203
2 Experiment 204
3 Results 204
4 Conclusion 206
References 206
Indirect techniques in nuclear astrophysics 207
1 Introduction 207
2 ANC method 207
3 Trojan Horse 212
4 Summary 217
References 217
Can the neutron-capture cross sections be measured with Coulomb dissociation? 218
1 Introduction 218
2 The method of Coulomb dissociation and its experimental di.culties 219
3 The experimental procedure 219
4 Results and discussion 220
References 221
Study of the 9Be(p, a)6Li reaction via the Trojan Horse Method 222
1 Introduction 222
2 The Trojan Horse Method 222
3 Experimental procedure 223
4 Data analysis 223
5 Conclusion 225
References 226
Re-evaluation of the low-energy Coulomb-dissociation cross section of 8B and the astrophysical S17 factor 227
1 Introduction 227
2 Theoretical calculations 227
3 Experimental procedures 228
4 Data reduction and results 228
5 The astrophysical S17 factor 231
6 Conclusions 232
References 232
Study of the 26Si(p, .)27P reaction through Coulomb dissociation of 27P 233
1 Introduction 233
2 Experiment 234
3 Result and discussion 235
4 Summary 236
References 236
Breakup of loosely bound nuclei as indirect method in nuclear astrophysics: 8B, 9C, 23Al 237
1 Introduction 237
2 The reaction model 238
3 Three particular cases 238
4 Conclusions 242
Relation between proton and neutron asymptotic normalizaion coe.cients for light mirror nuclei and its relevance for nuclear astrophysics 243
1 Introduction 243
2 Plane-Wave Impulse Approximation 244
3 The experiment 244
4 Data analysis and results 245
5 Conclusions 247
References 247
Indirect measurement of the 15N(p, a)12C reaction cross sectionthrough the Trojan-Horse Method 249
1 Introduction 249
2 The experiment 250
3 Results and discussion 253
References 254
6 Nuclear Structure Far from Stability 255
Nuclear structure far o. stability —Implications for nuclear astrophysics 256
1 Introduction 256
2 Spin-gap isomerism in the 100Sn region 257
3 Monopole driven shell structure in neutron-rich nuclei 259
4 Towards 78Ni 262
5 Shell structure along the r-path towards 262
6 Summary and conclusions 265
References 265
Relation between proton and neutron asymptotic normalization coe.cients for light mirror nuclei and its relevance for nuclear astrophysics 267
1 Introduction 267
2 Analytical formula 268
3 Single-particle model 269
4 Microscopic cluster model 270
5 Bound mirror pairs 270
6 Bound-unbound mirror pairs 272
7 Discussion and conclusions 273
References 274
A simple interpretation of global trends in the lowest levels of pand sd-shell nuclei 275
1 Introduction 275
2 The approach 276
3 Applications 278
4 Conclusions 280
References 280
Exploring the Na + 3n light nuclei via the (7Li, 7Be) reaction 281
1 Introduction 281
2 The (7Li, 7Be) CEX reaction 282
3 Nuclear structure model 283
4 Other explored Na + 3n systems 285
References 286
Equation of state of strongly interacting matter in compact stars 287
1 Introduction 287
2 Equation of state of compact stars matter 287
3 Signatures of quark matter in compact stars 291
4 Conclusions 292
References 292
Clustering in light nuclei in fragmentation above 1 A GeV 293
1 Introduction 293
2 Nuclear fragment jets 294
3 Fragmentation of 22Ne nuclei 295
4 Fragmentation of 14N nuclei 295
5 Fragmentation of 9Be nuclei 296
6 Charged topology of 8B fragmentation 297
7 Charged topology of 9C fragmentation 297
8 Conclusions 298
References 298
Effects of the particle-number projection on the isovector pairing energy 299
1 Introduction 299
2 BCS theory 300
3 Projection 300
4 Numerical results. Discussion 301
References 303
7 Rare-Ion-Beam Facilities and Experiments 305
Study of the N = 28 shell closure in the Ar isotopic chain 306
1 Introduction 306
2 Experimental methods 307
3 Experimental results 308
4 Determination of (n, .) rates from (d, p) reaction 309
5 Astrophysical implications 310
6 Conclusions 311
References 311
Status of the TRIUMF annular chamber for the tracking and identification of charged particles (TACTIC) 312
1 Introduction 312
2 The TACTIC chamber 312
3 The TACTIC test chamber. 313
4 GEANT4 simulation 314
5 Drift field and beam induced electrons 315
6 Data acquisition 316
7 Applications 316
8 Conclusions 317
References 317
Testing of the RIKEN-ATOMKI CsI(Tl) array in the study of 22,23O nuclear structure 318
1 Introduction 318
2 Characterization of the CsI(Tl) detectors 318
3 The commissioning experiment 320
4 Results and discussion 321
References 321
8 Perspectives of Nuclear Physics and Astrophysics 322
Nuclear astrophysics at the east drip line 323
1 Introduction 323
2 Experimental facilities in japan 324
3 The CRIB project at CNS 325
4 The direct measurement of the 14O(a, p)17F reaction 326
5 Search for proton resonances relevant to the early stage of the rp-process 327
6 Summary 327
References 328
Radiative electron capture —A tool to detect He++ in space 329
1 Introduction 329
2 Expected photon spectra due to Radiative Electron Capture in the plasma clouds 330
3 Summary and conclusions 331
References 331
AMS —A powerful tool for probing nucleosynthesis via long-lived radionuclides 332
1 Introduction 332
2 Accelerator mass spectrometry at the Vienna Environmental Research Accelerator facility 332
3 Applications of AMS related to astrophysics 334
4 Ca-measurements with VERA 335
5 Summary 336
References 337
Author index 338
Erscheint lt. Verlag | 31.12.2007 |
---|---|
Zusatzinfo | XVI, 349 p. |
Verlagsort | Berlin |
Sprache | englisch |
Themenwelt | Naturwissenschaften ► Physik / Astronomie ► Astronomie / Astrophysik |
Naturwissenschaften ► Physik / Astronomie ► Atom- / Kern- / Molekularphysik | |
Technik | |
Schlagworte | astrophysics • cross section • Electron Capture • Experiment • Hadron • Neutrino • Neutron • nuclear astrophysics • Nuclear data • Nucleosynthesis |
ISBN-10 | 3-540-32843-2 / 3540328432 |
ISBN-13 | 978-3-540-32843-8 / 9783540328438 |
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