<p>The continuum quasiparticle random phase approximation (CQRPA), which includes the Skyrme interaction for both ground- and excited-state calculations, is extended in a more consistent manner in the present work. The emergence, evolution, and origin of pygmy monopole strengths along the even–even Ni isotopes were investigated carefully within consistent Skyrme HF + BCS and CQRPA models. The SLy5 Skyrme interaction and density-dependent zero-range pairing interactions were adopted in the calculations. No pygmy monopole strength was observed in <InlineEquation ID="IEq1"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="41365_2025_1794_Article_IEq1.gif" Format="GIF" Height="11" Rendition="HTML" Resolution="72" Type="Linedraw" Width="34" /> </InlineMediaObject> <EquationSource Format="TEX">\(^{70-78}\)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mrow /> <mrow> <mn>70</mn> <mo>-</mo> <mn>78</mn> </mrow> </mmultiscripts> </math></EquationSource> </InlineEquation>Ni. However, pronounced pygmy monopole strengths are clearly observed in <InlineEquation ID="IEq2"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="41365_2025_1794_Article_IEq2.gif" Format="GIF" Height="11" Rendition="HTML" Resolution="72" Type="Linedraw" Width="34" /> </InlineMediaObject> <EquationSource Format="TEX">\(^{80-84}\)</EquationSource> <EquationSource Format="MATHML"><math> <mmultiscripts> <mrow /> <mrow /> <mrow> <mn>80</mn> <mo>-</mo> <mn>84</mn> </mrow> </mmultiscripts> </math></EquationSource> </InlineEquation>Ni, which are attributed mainly to the neutron excitations from weakly bound orbitals into the continuum. The neutron states involved in the pygmy monopole strength include 1<InlineEquation ID="IEq3"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="41365_2025_1794_Article_IEq3.gif" Format="GIF" Height="15" Rendition="HTML" Resolution="72" Type="Linedraw" Width="28" /> </InlineMediaObject> <EquationSource Format="TEX">\(g_{9/2}\)</EquationSource> <EquationSource Format="MATHML"><math> <msub> <mi>g</mi> <mrow> <mn>9</mn> <mo stretchy="false">/</mo> <mn>2</mn> </mrow> </msub> </math></EquationSource> </InlineEquation>, 2<InlineEquation ID="IEq4"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="41365_2025_1794_Article_IEq4.gif" Format="GIF" Height="20" Rendition="HTML" Resolution="72" Type="Linedraw" Width="28" /> </InlineMediaObject> <EquationSource Format="TEX">\(d_{5/2}\)</EquationSource> <EquationSource Format="MATHML"><math> <msub> <mi>d</mi> <mrow> <mn>5</mn> <mo stretchy="false">/</mo> <mn>2</mn> </mrow> </msub> </math></EquationSource> </InlineEquation>, 3<InlineEquation ID="IEq5"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="41365_2025_1794_Article_IEq5.gif" Format="GIF" Height="15" Rendition="HTML" Resolution="72" Type="Linedraw" Width="27" /> </InlineMediaObject> <EquationSource Format="TEX">\(s_{1/2}\)</EquationSource> <EquationSource Format="MATHML"><math> <msub> <mi>s</mi> <mrow> <mn>1</mn> <mo stretchy="false">/</mo> <mn>2</mn> </mrow> </msub> </math></EquationSource> </InlineEquation> and 2<InlineEquation ID="IEq6"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="41365_2025_1794_Article_IEq6.gif" Format="GIF" Height="20" Rendition="HTML" Resolution="72" Type="Linedraw" Width="28" /> </InlineMediaObject> <EquationSource Format="TEX">\(d_{3/2}\)</EquationSource> <EquationSource Format="MATHML"><math> <msub> <mi>d</mi> <mrow> <mn>3</mn> <mo stretchy="false">/</mo> <mn>2</mn> </mrow> </msub> </math></EquationSource> </InlineEquation>. We suggest that more efforts from experimental investigations of pygmy monopole resonance should be made to confirm or disprove the predictions from models in the future.</p>

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Emergence of pygmy monopole strength in neutron-rich nickel isotopes

  • Shuai Sun,
  • Ya-Lu Wang,
  • Miao Qi,
  • Rong An,
  • Li-Gang Cao,
  • Feng-Shou Zhang

摘要

The continuum quasiparticle random phase approximation (CQRPA), which includes the Skyrme interaction for both ground- and excited-state calculations, is extended in a more consistent manner in the present work. The emergence, evolution, and origin of pygmy monopole strengths along the even–even Ni isotopes were investigated carefully within consistent Skyrme HF + BCS and CQRPA models. The SLy5 Skyrme interaction and density-dependent zero-range pairing interactions were adopted in the calculations. No pygmy monopole strength was observed in \(^{70-78}\) 70 - 78 Ni. However, pronounced pygmy monopole strengths are clearly observed in \(^{80-84}\) 80 - 84 Ni, which are attributed mainly to the neutron excitations from weakly bound orbitals into the continuum. The neutron states involved in the pygmy monopole strength include 1 \(g_{9/2}\) g 9 / 2 , 2 \(d_{5/2}\) d 5 / 2 , 3 \(s_{1/2}\) s 1 / 2 and 2 \(d_{3/2}\) d 3 / 2 . We suggest that more efforts from experimental investigations of pygmy monopole resonance should be made to confirm or disprove the predictions from models in the future.