1978
DOI: 10.1088/0305-4616/4/7/016
|View full text |Cite
|
Sign up to set email alerts
|

g9/2isobaric analogue resonances in the56Fe(p,γ)57Co reaction

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
3
1
1

Citation Types

0
7
0

Year Published

1981
1981
2019
2019

Publication Types

Select...
5
3

Relationship

0
8

Authors

Journals

citations
Cited by 17 publications
(7 citation statements)
references
References 7 publications
0
7
0
Order By: Relevance
“…This includes effects due to the temperature dependence of the effective number of relativistic degrees of freedom g * (and of the analogous quantity defined via the entropy density rather than via the energy density of the radiation). Here we use the results of [47], which assumes free electroweak gauge and Higgs bosons, as appropriate for a smooth crossover electroweak transition [48][49][50]. Moreover, it uses results from lattice QCD around the QCD transition temperature, matched to a hadron resonance gas at lower temperatures [51,52].…”
Section: Introductionmentioning
confidence: 99%
“…This includes effects due to the temperature dependence of the effective number of relativistic degrees of freedom g * (and of the analogous quantity defined via the entropy density rather than via the energy density of the radiation). Here we use the results of [47], which assumes free electroweak gauge and Higgs bosons, as appropriate for a smooth crossover electroweak transition [48][49][50]. Moreover, it uses results from lattice QCD around the QCD transition temperature, matched to a hadron resonance gas at lower temperatures [51,52].…”
Section: Introductionmentioning
confidence: 99%
“…Some information on resonances in this energy range will be the subject of a future publication [11]. Using our value AEc=8,876+6keV, Fodor et al [12] have identified resonances at Ep=3,728 and 3,735keV in the 56Fe(p,y)STCo reaction as the split analogue of the 2,454 keV level in 57Fe.…”
Section: Analogue State Identificationmentioning
confidence: 81%
“…Numerical evolution -Though multi-oscillator solutions never collapse to form black holes, they can be unstable. Indeed, solutions such as boson stars [8,41,54,55] and oscillatons [7,56] form a subset of the multi-oscillator family and are known to be unstable to black hole formation for sufficiently large energies. In a sense, these unstable solutions would constitute regions of the islands of stability that are locally measure zero.…”
Section: Arxiv:190802296v1 [Hep-th] 6 Aug 2019mentioning
confidence: 99%