Loading…

Spontaneous Fission Previously Observed in a Mercury Source

PREVIOUSLY 1 , we have presented evidence for the possible existence of a superheavy element with atomic number 112. The principal evidence for the possible existence of this element was based on the observation of spontaneous fission in a mercury source separated from a tungsten target which had be...

Full description

Saved in:
Bibliographic Details
Published in:Nature (London) 1971-01, Vol.234 (5326), p.212-215
Main Authors: MARINOV, A, BATTY, C. J, KILVINGTON, A. I, WEIL, J. L, FRIEDMAN, A. M, NEWTON, G. W. A, ROBINSON, V. J, HEMINGWAY, J. D, MATHER, D. S
Format: Article
Language:English
Subjects:
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by cdi_FETCH-LOGICAL-c309t-75c8def9e9a1c34ccb0495d70e6151f81af2533e042c2ffc357b07d8743abdb13
cites cdi_FETCH-LOGICAL-c309t-75c8def9e9a1c34ccb0495d70e6151f81af2533e042c2ffc357b07d8743abdb13
container_end_page 215
container_issue 5326
container_start_page 212
container_title Nature (London)
container_volume 234
creator MARINOV, A
BATTY, C. J
KILVINGTON, A. I
WEIL, J. L
FRIEDMAN, A. M
NEWTON, G. W. A
ROBINSON, V. J
HEMINGWAY, J. D
MATHER, D. S
description PREVIOUSLY 1 , we have presented evidence for the possible existence of a superheavy element with atomic number 112. The principal evidence for the possible existence of this element was based on the observation of spontaneous fission in a mercury source separated from a tungsten target which had been irradiated by 24 GeV protons. Spontaneous fission activity was observed, using polycarbonate foils, in mercury sources separated from two tungsten targets. These latter are identified by the symbols W2 and W3. In the case of the W3 source the proton dose was probably less than for W2 and also only about 30% of the mercury added as carrier was recovered in the final source (as measured by colorimetric techniques). The observed fission activity was smaller than that observed with the W2 source. In the latter case (W2) the measured activity was originally about three fissions/day and all experimental work reported here has been carried out with this sample.
doi_str_mv 10.1038/234212b0
format article
fullrecord <record><control><sourceid>nature_cross</sourceid><recordid>TN_cdi_crossref_primary_10_1038_234212b0</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>234212b0</sourcerecordid><originalsourceid>FETCH-LOGICAL-c309t-75c8def9e9a1c34ccb0495d70e6151f81af2533e042c2ffc357b07d8743abdb13</originalsourceid><addsrcrecordid>eNptz19LwzAUBfAgCtYp-Akkj_pQvfnTJsUnGU6FyYTpc0nTG-mY6UjaQb-9leqefLpw-XE4h5BLBrcMhL7jQnLGKzgiCZMqT2Wu1TFJALhOQYv8lJzFuAGAjCmZkPv1rvWd8dj2kS6aGJvW07eA-2Z8bAe6qiKGPda08dTQVwy2DwNdt32weE5OnNlGvPi9M_KxeHyfP6fL1dPL_GGZWgFFl6rM6hpdgYVhVkhrK5BFVivAnGXMaWYcz4RAkNxy56zIVAWq1koKU9UVEzNyPeXa0MYY0JW70HyZMJQMyp_R5d_okd5MNI7Ef2IoN2NVP7b7z15N1puuD3gIPYBv5Q5gnQ</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Spontaneous Fission Previously Observed in a Mercury Source</title><source>Nature</source><creator>MARINOV, A ; BATTY, C. J ; KILVINGTON, A. I ; WEIL, J. L ; FRIEDMAN, A. M ; NEWTON, G. W. A ; ROBINSON, V. J ; HEMINGWAY, J. D ; MATHER, D. S</creator><creatorcontrib>MARINOV, A ; BATTY, C. J ; KILVINGTON, A. I ; WEIL, J. L ; FRIEDMAN, A. M ; NEWTON, G. W. A ; ROBINSON, V. J ; HEMINGWAY, J. D ; MATHER, D. S</creatorcontrib><description>PREVIOUSLY 1 , we have presented evidence for the possible existence of a superheavy element with atomic number 112. The principal evidence for the possible existence of this element was based on the observation of spontaneous fission in a mercury source separated from a tungsten target which had been irradiated by 24 GeV protons. Spontaneous fission activity was observed, using polycarbonate foils, in mercury sources separated from two tungsten targets. These latter are identified by the symbols W2 and W3. In the case of the W3 source the proton dose was probably less than for W2 and also only about 30% of the mercury added as carrier was recovered in the final source (as measured by colorimetric techniques). The observed fission activity was smaller than that observed with the W2 source. In the latter case (W2) the measured activity was originally about three fissions/day and all experimental work reported here has been carried out with this sample.</description><identifier>ISSN: 0028-0836</identifier><identifier>EISSN: 1476-4687</identifier><identifier>DOI: 10.1038/234212b0</identifier><language>eng</language><publisher>London: Nature Publishing Group UK</publisher><subject>Humanities and Social Sciences ; letter ; multidisciplinary ; Science ; Science (multidisciplinary)</subject><ispartof>Nature (London), 1971-01, Vol.234 (5326), p.212-215</ispartof><rights>Springer Nature Limited 1971</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c309t-75c8def9e9a1c34ccb0495d70e6151f81af2533e042c2ffc357b07d8743abdb13</citedby><cites>FETCH-LOGICAL-c309t-75c8def9e9a1c34ccb0495d70e6151f81af2533e042c2ffc357b07d8743abdb13</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,2727,27924,27925</link.rule.ids></links><search><creatorcontrib>MARINOV, A</creatorcontrib><creatorcontrib>BATTY, C. J</creatorcontrib><creatorcontrib>KILVINGTON, A. I</creatorcontrib><creatorcontrib>WEIL, J. L</creatorcontrib><creatorcontrib>FRIEDMAN, A. M</creatorcontrib><creatorcontrib>NEWTON, G. W. A</creatorcontrib><creatorcontrib>ROBINSON, V. J</creatorcontrib><creatorcontrib>HEMINGWAY, J. D</creatorcontrib><creatorcontrib>MATHER, D. S</creatorcontrib><title>Spontaneous Fission Previously Observed in a Mercury Source</title><title>Nature (London)</title><addtitle>Nature</addtitle><description>PREVIOUSLY 1 , we have presented evidence for the possible existence of a superheavy element with atomic number 112. The principal evidence for the possible existence of this element was based on the observation of spontaneous fission in a mercury source separated from a tungsten target which had been irradiated by 24 GeV protons. Spontaneous fission activity was observed, using polycarbonate foils, in mercury sources separated from two tungsten targets. These latter are identified by the symbols W2 and W3. In the case of the W3 source the proton dose was probably less than for W2 and also only about 30% of the mercury added as carrier was recovered in the final source (as measured by colorimetric techniques). The observed fission activity was smaller than that observed with the W2 source. In the latter case (W2) the measured activity was originally about three fissions/day and all experimental work reported here has been carried out with this sample.</description><subject>Humanities and Social Sciences</subject><subject>letter</subject><subject>multidisciplinary</subject><subject>Science</subject><subject>Science (multidisciplinary)</subject><issn>0028-0836</issn><issn>1476-4687</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1971</creationdate><recordtype>article</recordtype><recordid>eNptz19LwzAUBfAgCtYp-Akkj_pQvfnTJsUnGU6FyYTpc0nTG-mY6UjaQb-9leqefLpw-XE4h5BLBrcMhL7jQnLGKzgiCZMqT2Wu1TFJALhOQYv8lJzFuAGAjCmZkPv1rvWd8dj2kS6aGJvW07eA-2Z8bAe6qiKGPda08dTQVwy2DwNdt32weE5OnNlGvPi9M_KxeHyfP6fL1dPL_GGZWgFFl6rM6hpdgYVhVkhrK5BFVivAnGXMaWYcz4RAkNxy56zIVAWq1koKU9UVEzNyPeXa0MYY0JW70HyZMJQMyp_R5d_okd5MNI7Ef2IoN2NVP7b7z15N1puuD3gIPYBv5Q5gnQ</recordid><startdate>19710101</startdate><enddate>19710101</enddate><creator>MARINOV, A</creator><creator>BATTY, C. J</creator><creator>KILVINGTON, A. I</creator><creator>WEIL, J. L</creator><creator>FRIEDMAN, A. M</creator><creator>NEWTON, G. W. A</creator><creator>ROBINSON, V. J</creator><creator>HEMINGWAY, J. D</creator><creator>MATHER, D. S</creator><general>Nature Publishing Group UK</general><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>19710101</creationdate><title>Spontaneous Fission Previously Observed in a Mercury Source</title><author>MARINOV, A ; BATTY, C. J ; KILVINGTON, A. I ; WEIL, J. L ; FRIEDMAN, A. M ; NEWTON, G. W. A ; ROBINSON, V. J ; HEMINGWAY, J. D ; MATHER, D. S</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c309t-75c8def9e9a1c34ccb0495d70e6151f81af2533e042c2ffc357b07d8743abdb13</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1971</creationdate><topic>Humanities and Social Sciences</topic><topic>letter</topic><topic>multidisciplinary</topic><topic>Science</topic><topic>Science (multidisciplinary)</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>MARINOV, A</creatorcontrib><creatorcontrib>BATTY, C. J</creatorcontrib><creatorcontrib>KILVINGTON, A. I</creatorcontrib><creatorcontrib>WEIL, J. L</creatorcontrib><creatorcontrib>FRIEDMAN, A. M</creatorcontrib><creatorcontrib>NEWTON, G. W. A</creatorcontrib><creatorcontrib>ROBINSON, V. J</creatorcontrib><creatorcontrib>HEMINGWAY, J. D</creatorcontrib><creatorcontrib>MATHER, D. S</creatorcontrib><collection>CrossRef</collection><jtitle>Nature (London)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>MARINOV, A</au><au>BATTY, C. J</au><au>KILVINGTON, A. I</au><au>WEIL, J. L</au><au>FRIEDMAN, A. M</au><au>NEWTON, G. W. A</au><au>ROBINSON, V. J</au><au>HEMINGWAY, J. D</au><au>MATHER, D. S</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Spontaneous Fission Previously Observed in a Mercury Source</atitle><jtitle>Nature (London)</jtitle><stitle>Nature</stitle><date>1971-01-01</date><risdate>1971</risdate><volume>234</volume><issue>5326</issue><spage>212</spage><epage>215</epage><pages>212-215</pages><issn>0028-0836</issn><eissn>1476-4687</eissn><abstract>PREVIOUSLY 1 , we have presented evidence for the possible existence of a superheavy element with atomic number 112. The principal evidence for the possible existence of this element was based on the observation of spontaneous fission in a mercury source separated from a tungsten target which had been irradiated by 24 GeV protons. Spontaneous fission activity was observed, using polycarbonate foils, in mercury sources separated from two tungsten targets. These latter are identified by the symbols W2 and W3. In the case of the W3 source the proton dose was probably less than for W2 and also only about 30% of the mercury added as carrier was recovered in the final source (as measured by colorimetric techniques). The observed fission activity was smaller than that observed with the W2 source. In the latter case (W2) the measured activity was originally about three fissions/day and all experimental work reported here has been carried out with this sample.</abstract><cop>London</cop><pub>Nature Publishing Group UK</pub><doi>10.1038/234212b0</doi><tpages>4</tpages></addata></record>
fulltext fulltext
identifier ISSN: 0028-0836
ispartof Nature (London), 1971-01, Vol.234 (5326), p.212-215
issn 0028-0836
1476-4687
language eng
recordid cdi_crossref_primary_10_1038_234212b0
source Nature
subjects Humanities and Social Sciences
letter
multidisciplinary
Science
Science (multidisciplinary)
title Spontaneous Fission Previously Observed in a Mercury Source
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-27T11%3A19%3A31IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-nature_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Spontaneous%20Fission%20Previously%20Observed%20in%20a%20Mercury%20Source&rft.jtitle=Nature%20(London)&rft.au=MARINOV,%20A&rft.date=1971-01-01&rft.volume=234&rft.issue=5326&rft.spage=212&rft.epage=215&rft.pages=212-215&rft.issn=0028-0836&rft.eissn=1476-4687&rft_id=info:doi/10.1038/234212b0&rft_dat=%3Cnature_cross%3E234212b0%3C/nature_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c309t-75c8def9e9a1c34ccb0495d70e6151f81af2533e042c2ffc357b07d8743abdb13%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true