FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2135648209> ?p ?o ?g. }

• W2135648209 abstract "The best examples of halo nuclei, exotic systems with a diffuse nuclear cloud surrounding a tightly bound core, are found in the light, neutron-rich region, where the halo neutrons experience only weak binding and a weak, or no, potential barrier. Modern direct-reaction measurement techniques provide powerful probes of the structure of exotic nuclei. Despite more than four decades of these studies on the benchmark one-neutron halo nucleus 11Be, the spectroscopic factors for the two bound states remain poorly constrained. In the present work, the 10Be(d,​p) reaction has been used in inverse kinematics at four beam energies to study the structure of 11Be. The spectroscopic factors extracted using the adiabatic model were found to be consistent across the four measurements and were largely insensitive to the optical potential used. The extracted spectroscopic factor for a neutron in an nℓj=2s(1/2) state coupled to the ground state of 10Be is 0.71(5). For the first excited state at 0.32 MeV, a spectroscopic factor of 0.62(4) is found for the halo neutron in a 1p(1/2) state." @default.
• W2135648209 created "2016-06-24" @default.
• W2135648209 creator A5000060864 @default.
• W2135648209 creator A5002479734 @default.
• W2135648209 creator A5008706482 @default.
• W2135648209 creator A5012042206 @default.
• W2135648209 creator A5012920531 @default.
• W2135648209 creator A5013540904 @default.
• W2135648209 creator A5014247682 @default.
• W2135648209 creator A5014780786 @default.
• W2135648209 creator A5017021374 @default.
• W2135648209 creator A5021627861 @default.
• W2135648209 creator A5029605572 @default.
• W2135648209 creator A5033041764 @default.
• W2135648209 creator A5033081403 @default.
• W2135648209 creator A5033257466 @default.
• W2135648209 creator A5033475921 @default.
• W2135648209 creator A5036605912 @default.
• W2135648209 creator A5045829106 @default.
• W2135648209 creator A5048133037 @default.
• W2135648209 creator A5048247549 @default.
• W2135648209 creator A5049448202 @default.
• W2135648209 creator A5056598336 @default.
• W2135648209 creator A5064915382 @default.
• W2135648209 creator A5069645645 @default.
• W2135648209 creator A5069756433 @default.
• W2135648209 creator A5071737800 @default.
• W2135648209 creator A5072239908 @default.
• W2135648209 creator A5074815564 @default.
• W2135648209 creator A5077194551 @default.
• W2135648209 creator A5078847237 @default.
• W2135648209 creator A5078995798 @default.
• W2135648209 creator A5080019559 @default.
• W2135648209 creator A5083516196 @default.
• W2135648209 date "2012-05-08" @default.
• W2135648209 modified "2023-10-05" @default.
• W2135648209 title "Halo Nucleus<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts /><mml:none /><mml:mn>11</mml:mn></mml:mmultiscripts></mml:math>: A Spectroscopic Study via Neutron Transfer" @default.
• W2135648209 cites W156801620 @default.
• W2135648209 cites W1619926894 @default.
• W2135648209 cites W1979832929 @default.
• W2135648209 cites W1981123452 @default.
• W2135648209 cites W1987028746 @default.
• W2135648209 cites W1990052327 @default.
• W2135648209 cites W1990247359 @default.
• W2135648209 cites W2002580335 @default.
• W2135648209 cites W2022857785 @default.
• W2135648209 cites W2027768099 @default.
• W2135648209 cites W2028701003 @default.
• W2135648209 cites W2033819022 @default.
• W2135648209 cites W2036728050 @default.
• W2135648209 cites W2039155201 @default.
• W2135648209 cites W2040359393 @default.
• W2135648209 cites W2042497539 @default.
• W2135648209 cites W2045141240 @default.
• W2135648209 cites W2074726287 @default.
• W2135648209 cites W2074752748 @default.
• W2135648209 cites W2075009846 @default.
• W2135648209 cites W2075264401 @default.
• W2135648209 cites W2076779267 @default.
• W2135648209 cites W2082876765 @default.
• W2135648209 cites W2083136656 @default.
• W2135648209 cites W2084282902 @default.
• W2135648209 cites W2089594658 @default.
• W2135648209 cites W2095439927 @default.
• W2135648209 cites W2098592324 @default.
• W2135648209 cites W2110285102 @default.
• W2135648209 cites W2124319596 @default.
• W2135648209 cites W2141987782 @default.
• W2135648209 cites W2614802106 @default.
• W2135648209 cites W2803908589 @default.
• W2135648209 cites W3124817923 @default.
• W2135648209 cites W48027786 @default.
• W2135648209 doi "https://doi.org/10.1103/physrevlett.108.192701" @default.
• W2135648209 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/23003029" @default.
• W2135648209 hasPublicationYear "2012" @default.
• W2135648209 type Work @default.
• W2135648209 sameAs 2135648209 @default.
• W2135648209 citedByCount "81" @default.
• W2135648209 countsByYear W21356482092012 @default.
• W2135648209 countsByYear W21356482092013 @default.
• W2135648209 countsByYear W21356482092014 @default.
• W2135648209 countsByYear W21356482092015 @default.
• W2135648209 countsByYear W21356482092016 @default.
• W2135648209 countsByYear W21356482092017 @default.
• W2135648209 countsByYear W21356482092018 @default.
• W2135648209 countsByYear W21356482092019 @default.
• W2135648209 countsByYear W21356482092020 @default.
• W2135648209 countsByYear W21356482092021 @default.
• W2135648209 countsByYear W21356482092022 @default.
• W2135648209 countsByYear W21356482092023 @default.
• W2135648209 crossrefType "journal-article" @default.
• W2135648209 hasAuthorship W2135648209A5000060864 @default.
• W2135648209 hasAuthorship W2135648209A5002479734 @default.
• W2135648209 hasAuthorship W2135648209A5008706482 @default.
• W2135648209 hasAuthorship W2135648209A5012042206 @default.
• W2135648209 hasAuthorship W2135648209A5012920531 @default.
• W2135648209 hasAuthorship W2135648209A5013540904 @default.
• W2135648209 hasAuthorship W2135648209A5014247682 @default.
• W2135648209 hasAuthorship W2135648209A5014780786 @default.
• W2135648209 hasAuthorship W2135648209A5017021374 @default.

• next