{"id":223,"date":"2017-01-26T10:28:55","date_gmt":"2017-01-26T08:28:55","guid":{"rendered":"http:\/\/magneticmoments.info\/wp\/?p=223"},"modified":"2017-01-26T10:32:25","modified_gmt":"2017-01-26T08:32:25","slug":"paper-the-orbital-g-factor-and-related-sum-rules","status":"publish","type":"post","link":"https:\/\/magneticmoments.info\/wp\/?p=223","title":{"rendered":"[paper] The orbital g-factor and related sum rules"},"content":{"rendered":"<p><em>The orbital g-factor and related sum rules<\/em><\/p>\n<p>Wolfgang Bentz and Akito Arima<\/p>\n<p>doi: <a href=\"https:\/\/doi.org\/10.1007\/s11433-010-4224-6\">10.1007\/s11433-010-4224-6<\/a><\/p>\n<p>The renormalization of the orbital g-factor in nuclei is discussed on the basis of gauge invariance. The relation of the orbital g-factor to the integrated E1 photoabsorption cross section is reviewed, and its relation to the M1 sum rule for the scissors mode of deformed nuclei is examined.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>The orbital g-factor and related sum rules Wolfgang Bentz and Akito Arima doi: 10.1007\/s11433-010-4224-6 The renormalization of the orbital g-factor in nuclei is discussed on the basis of gauge invariance. The relation of the orbital g-factor to the integrated E1&#46;&#46;&#46;<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"jetpack_post_was_ever_published":false,"jetpack_publicize_message":"","jetpack_is_tweetstorm":false,"jetpack_publicize_feature_enabled":true,"jetpack_social_post_already_shared":true,"jetpack_social_options":{"image_generator_settings":{"template":"highway","enabled":false}}},"categories":[1,4],"tags":[85],"jetpack_publicize_connections":[],"jetpack_featured_media_url":"","jetpack_sharing_enabled":true,"jetpack_shortlink":"https:\/\/wp.me\/p6YIb0-3B","jetpack-related-posts":[{"id":115,"url":"https:\/\/magneticmoments.info\/wp\/?p=115","url_meta":{"origin":223,"position":0},"title":"[paper] Structure of the Sr-Zr isotopes near and at the magic N=50 shell from g-factor and lifetime measurements in8840Zr and 84,86,8838Sr","date":"Apr 30, 2012","format":false,"excerpt":"Structure of the Sr-Zr isotopes near and at the magic N=50 shell from g-factor and lifetime measurements in8840Zr and 84,86,8838Sr G. 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The isoscalar spin gyromagnetic ratios gsIS of nuclei with one nucleon or hole outside\u2026","rel":"","context":"In &quot;g factor&quot;","img":{"alt_text":"","src":"https:\/\/i0.wp.com\/mertzimekis.gr\/home\/wp-content\/uploads\/2019\/01\/GT-1.png?resize=350%2C200","width":350,"height":200},"classes":[]},{"id":151,"url":"https:\/\/magneticmoments.info\/wp\/?p=151","url_meta":{"origin":223,"position":2},"title":"[paper] The energy-weighted sum rule and the nuclear radius","date":"Oct 2, 2015","format":false,"excerpt":"The energy-weighted sum rule and the nuclear radius Hans Peter Schr\u00f6der doi: 10.1140\/epja\/i2015-15109-9 The energy-weighted integrated cross-section for photon absorption --known as sum rule \u03c3\u22121 -- is under certain conditions proportional to the mean square nuclear radius (Levinger, Bethe (Phys. Rev. 78, 115 (1950))). Due to the energy weight factor\u2026","rel":"","context":"In &quot;radii&quot;","img":{"alt_text":"","src":"","width":0,"height":0},"classes":[]},{"id":76,"url":"https:\/\/magneticmoments.info\/wp\/?p=76","url_meta":{"origin":223,"position":3},"title":"[paper] Magnetic moments of the first excited 2+ states in the semi-magic 112,114,116,122,124Sn isotopes","date":"Jul 19, 2011","format":false,"excerpt":"Magnetic moments of the first excited 2+ states in the semi-magic 112,114,116,122,124Sn isotopes J. Walker et al. doi: 10.1103\/PhysRevC.84.014319 The g factors of the first excited 2+ states in the 112,114,116,122,124Sn isotopes have been measured with high accuracy using the transient field technique in combination with Coulomb excitation in inverse\u2026","rel":"","context":"In &quot;experiment&quot;","img":{"alt_text":"","src":"","width":0,"height":0},"classes":[]},{"id":45,"url":"https:\/\/magneticmoments.info\/wp\/?p=45","url_meta":{"origin":223,"position":4},"title":"[paper] Shape coexistence near the N=38 shell gap: Magnetic moment of the 981.6 keV J&pi;=8+ level in 72As","date":"Oct 20, 2010","format":false,"excerpt":"Shape coexistence near the N=38 shell gap: Magnetic moment of the 981.6 keV J\u03c0=8+ level in 72As D. Pantelic&abreve; et al. doi: 10.1103\/PhysRevC.82.044313 We report on the first determination of the magnetic moment of the 981.1 keV, J\u03c0=8+ level in 72As, a nucleus that belongs to the A\u224870 mass region\u2026","rel":"","context":"In &quot;experiment&quot;","img":{"alt_text":"","src":"","width":0,"height":0},"classes":[]},{"id":264,"url":"https:\/\/magneticmoments.info\/wp\/?p=264","url_meta":{"origin":223,"position":5},"title":"[paper] Perturbed angular distributions with LaBr3  detectors: The $g$ factor of the first 10$^+$  state in $^{110}$Cd reexamined","date":"Nov 29, 2017","format":false,"excerpt":"Perturbed angular distributions with LaBr3 \u00a0detectors: The g factor of the first 10+ \u00a0state in 110Cd reexamined T.J. Gray et al. doi: 10.1103\/PhysRevC.96.054332 The time differential perturbed angular distribution technique with LaBr3 detectors has been applied to the I\u03c0=11\/2\u2212 isomeric state (Ex = 846 keV, \u03c4=107 ns) in 107Cd, which\u2026","rel":"","context":"In &quot;g factor&quot;","img":{"alt_text":"","src":"","width":0,"height":0},"classes":[]}],"_links":{"self":[{"href":"https:\/\/magneticmoments.info\/wp\/index.php?rest_route=\/wp\/v2\/posts\/223"}],"collection":[{"href":"https:\/\/magneticmoments.info\/wp\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/magneticmoments.info\/wp\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/magneticmoments.info\/wp\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/magneticmoments.info\/wp\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=223"}],"version-history":[{"count":2,"href":"https:\/\/magneticmoments.info\/wp\/index.php?rest_route=\/wp\/v2\/posts\/223\/revisions"}],"predecessor-version":[{"id":227,"href":"https:\/\/magneticmoments.info\/wp\/index.php?rest_route=\/wp\/v2\/posts\/223\/revisions\/227"}],"wp:attachment":[{"href":"https:\/\/magneticmoments.info\/wp\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=223"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/magneticmoments.info\/wp\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=223"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/magneticmoments.info\/wp\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=223"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}