Special features of the structure of the beta-stability line for nuclei
The mass-number ( A ) dependence Z β ( A ) for nuclei lying on the beta-stability line (BSL) is calculated for A and Z values in the ranges of A = 2–258 and Z = 1–100, respectively. The calculated values are compared with experimental data. The deviations Δ Z = Z expt − Z β are analyzed. This analys...
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| Veröffentlicht in: | Physics of atomic nuclei 2017-07, Vol.80 (4), p.623-630 |
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| container_title | Physics of atomic nuclei |
| container_volume | 80 |
| creator | Lutostansky, Yu. S. Tikhonov, V. N. |
| description | The mass-number (
A
) dependence
Z
β
(
A
) for nuclei lying on the beta-stability line (BSL) is calculated for
A
and
Z
values in the ranges of
A
= 2–258 and
Z
= 1–100, respectively. The calculated values are compared with experimental data. The deviations Δ
Z
=
Z
expt
−
Z
β
are analyzed. This analysis of Δ
Z
reveals that there are three regions of
A
values in which the
A
dependence of Δ
Z
is parabolic. The possible forms of the A dependence of ΔZ are analyzed, and it is shown that the majority of nuclei belong to several parabolas simultaneously. |
| doi_str_mv | 10.1134/S106377881703019X |
| format | Article |
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A
) dependence
Z
β
(
A
) for nuclei lying on the beta-stability line (BSL) is calculated for
A
and
Z
values in the ranges of
A
= 2–258 and
Z
= 1–100, respectively. The calculated values are compared with experimental data. The deviations Δ
Z
=
Z
expt
−
Z
β
are analyzed. This analysis of Δ
Z
reveals that there are three regions of
A
values in which the
A
dependence of Δ
Z
is parabolic. The possible forms of the A dependence of ΔZ are analyzed, and it is shown that the majority of nuclei belong to several parabolas simultaneously.</description><identifier>ISSN: 1063-7788</identifier><identifier>EISSN: 1562-692X</identifier><identifier>DOI: 10.1134/S106377881703019X</identifier><language>eng</language><publisher>Moscow: Pleiades Publishing</publisher><subject>COMPARATIVE EVALUATIONS ; MASS NUMBER ; Mathematical analysis ; NUCLEAR PHYSICS AND RADIATION PHYSICS ; NUCLEI ; PARABOLAS ; Particle and Nuclear Physics ; Physics ; Physics and Astronomy ; STABILITY ; Structural stability</subject><ispartof>Physics of atomic nuclei, 2017-07, Vol.80 (4), p.623-630</ispartof><rights>Pleiades Publishing, Ltd. 2017</rights><rights>Copyright Springer Science & Business Media 2017</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c344t-f096ab2d8716a2b2bd1a4f84c5623fa7b2c673479fe765e25a10dafec8209693</citedby><cites>FETCH-LOGICAL-c344t-f096ab2d8716a2b2bd1a4f84c5623fa7b2c673479fe765e25a10dafec8209693</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1134/S106377881703019X$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1134/S106377881703019X$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>230,314,776,780,881,27903,27904,41467,42536,51298</link.rule.ids><backlink>$$Uhttps://www.osti.gov/biblio/22759683$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Lutostansky, Yu. S.</creatorcontrib><creatorcontrib>Tikhonov, V. N.</creatorcontrib><title>Special features of the structure of the beta-stability line for nuclei</title><title>Physics of atomic nuclei</title><addtitle>Phys. Atom. Nuclei</addtitle><description>The mass-number (
A
) dependence
Z
β
(
A
) for nuclei lying on the beta-stability line (BSL) is calculated for
A
and
Z
values in the ranges of
A
= 2–258 and
Z
= 1–100, respectively. The calculated values are compared with experimental data. The deviations Δ
Z
=
Z
expt
−
Z
β
are analyzed. This analysis of Δ
Z
reveals that there are three regions of
A
values in which the
A
dependence of Δ
Z
is parabolic. The possible forms of the A dependence of ΔZ are analyzed, and it is shown that the majority of nuclei belong to several parabolas simultaneously.</description><subject>COMPARATIVE EVALUATIONS</subject><subject>MASS NUMBER</subject><subject>Mathematical analysis</subject><subject>NUCLEAR PHYSICS AND RADIATION PHYSICS</subject><subject>NUCLEI</subject><subject>PARABOLAS</subject><subject>Particle and Nuclear Physics</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>STABILITY</subject><subject>Structural stability</subject><issn>1063-7788</issn><issn>1562-692X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2017</creationdate><recordtype>article</recordtype><recordid>eNp1UMtKAzEUDaJgrX6AuwHXo7nJTDKzlOILCi7aRXchk97YlHFSk8yif29KFQVxdS_nxeEQcg30FoBXdwuggkvZNCApp9CuTsgEasFK0bLVaf4zXR74c3IR45ZSgKamE_K02KFxui8s6jQGjIW3RdpgEVMYzQH5BjpMuoxJd653aV_0bsDC-lAMo-nRXZIzq_uIV193SpaPD8vZczl_fXqZ3c9Lw6sqlZa2Qnds3UgQmnWsW4OubFOZXJVbLTtmhOSVbC1KUSOrNdC1tmgalp0tn5KbY6yPyaloXEKzMX4Y0CTFmKxb0fAf1S74jxFjUls_hiH3UtByVlEpa5ZVcFSZ4GMMaNUuuHcd9gqoOoyq_oyaPezoiVk7vGH4lfyv6RNw63f6</recordid><startdate>20170701</startdate><enddate>20170701</enddate><creator>Lutostansky, Yu. S.</creator><creator>Tikhonov, V. N.</creator><general>Pleiades Publishing</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>OTOTI</scope></search><sort><creationdate>20170701</creationdate><title>Special features of the structure of the beta-stability line for nuclei</title><author>Lutostansky, Yu. S. ; Tikhonov, V. N.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c344t-f096ab2d8716a2b2bd1a4f84c5623fa7b2c673479fe765e25a10dafec8209693</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2017</creationdate><topic>COMPARATIVE EVALUATIONS</topic><topic>MASS NUMBER</topic><topic>Mathematical analysis</topic><topic>NUCLEAR PHYSICS AND RADIATION PHYSICS</topic><topic>NUCLEI</topic><topic>PARABOLAS</topic><topic>Particle and Nuclear Physics</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>STABILITY</topic><topic>Structural stability</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Lutostansky, Yu. S.</creatorcontrib><creatorcontrib>Tikhonov, V. N.</creatorcontrib><collection>CrossRef</collection><collection>OSTI.GOV</collection><jtitle>Physics of atomic nuclei</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Lutostansky, Yu. S.</au><au>Tikhonov, V. N.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Special features of the structure of the beta-stability line for nuclei</atitle><jtitle>Physics of atomic nuclei</jtitle><stitle>Phys. Atom. Nuclei</stitle><date>2017-07-01</date><risdate>2017</risdate><volume>80</volume><issue>4</issue><spage>623</spage><epage>630</epage><pages>623-630</pages><issn>1063-7788</issn><eissn>1562-692X</eissn><abstract>The mass-number (
A
) dependence
Z
β
(
A
) for nuclei lying on the beta-stability line (BSL) is calculated for
A
and
Z
values in the ranges of
A
= 2–258 and
Z
= 1–100, respectively. The calculated values are compared with experimental data. The deviations Δ
Z
=
Z
expt
−
Z
β
are analyzed. This analysis of Δ
Z
reveals that there are three regions of
A
values in which the
A
dependence of Δ
Z
is parabolic. The possible forms of the A dependence of ΔZ are analyzed, and it is shown that the majority of nuclei belong to several parabolas simultaneously.</abstract><cop>Moscow</cop><pub>Pleiades Publishing</pub><doi>10.1134/S106377881703019X</doi><tpages>8</tpages></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 1063-7788 |
| ispartof | Physics of atomic nuclei, 2017-07, Vol.80 (4), p.623-630 |
| issn | 1063-7788 1562-692X |
| language | eng |
| recordid | cdi_osti_scitechconnect_22759683 |
| source | Springer Nature - Complete Springer Journals |
| subjects | COMPARATIVE EVALUATIONS MASS NUMBER Mathematical analysis NUCLEAR PHYSICS AND RADIATION PHYSICS NUCLEI PARABOLAS Particle and Nuclear Physics Physics Physics and Astronomy STABILITY Structural stability |
| title | Special features of the structure of the beta-stability line for nuclei |
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