AD 775 pulse of cosmogenic radionuclides production as imprint of a Galactic gamma-ray burst

We suggest an explanation of a sharp increase in the abundance of cosmogenic radiocarbon found in tree rings dated AD 775. The increase could originate from high-energy irradiation of the atmosphere by a Galactic gamma-ray burst. We argue that, unlike a cosmic ray event, a gamma-ray burst does not n...

Full description

Saved in:
Bibliographic Details
Published in:Monthly notices of the Royal Astronomical Society 2013-11, Vol.435 (4), p.2878-2884
Main Authors: Pavlov, A. K., Blinov, A. V., Konstantinov, A. N., Ostryakov, V. M., Vasilyev, G. I., Vdovina, M. A., Volkov, P. A.
Format: Article
Language:English
Subjects:
Astrophysics
Gamma ray astronomy
Protons
Star & galaxy formation
Citations: Items that this one cites
Items that cite this one
Online Access:Request full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by cdi_FETCH-LOGICAL-c403t-9776ccabd7319b55d41b8966432d152485b9b0f4d3f95912560239ca5a7381fb3
cites cdi_FETCH-LOGICAL-c403t-9776ccabd7319b55d41b8966432d152485b9b0f4d3f95912560239ca5a7381fb3
container_end_page 2884
container_issue 4
container_start_page 2878
container_title Monthly notices of the Royal Astronomical Society
container_volume 435
creator Pavlov, A. K.
Blinov, A. V.
Konstantinov, A. N.
Ostryakov, V. M.
Vasilyev, G. I.
Vdovina, M. A.
Volkov, P. A.
description We suggest an explanation of a sharp increase in the abundance of cosmogenic radiocarbon found in tree rings dated AD 775. The increase could originate from high-energy irradiation of the atmosphere by a Galactic gamma-ray burst. We argue that, unlike a cosmic ray event, a gamma-ray burst does not necessarily result in a substantial increase in long-lived 10Be atmospheric production. At the same time, the 36Cl nuclide would be generated in the amounts detectable in the corresponding ice-core samples from Greenland and Antarctica. These peculiar features allow experimental discrimination of nuclide effects caused by gamma-ray bursts and by powerful proton events.
doi_str_mv 10.1093/mnras/stt1468
format article
fullrecord <record><control><sourceid>proquest_TOX</sourceid><recordid>TN_cdi_proquest_journals_1442997625</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><oup_id>10.1093/mnras/stt1468</oup_id><sourcerecordid>3103098901</sourcerecordid><originalsourceid>FETCH-LOGICAL-c403t-9776ccabd7319b55d41b8966432d152485b9b0f4d3f95912560239ca5a7381fb3</originalsourceid><addsrcrecordid>eNqFkL1PwzAQxS0EEqUwsltiYTH1t-OxKlCQKrHAhhRdnKRK1cTBdob-97i0O9NJd7979-4hdM_oE6NWLPohQFzElJjUxQWaMaEV4VbrSzSjVChSGMau0U2MO0qpFFzP0PfyGRuj8DjtY4N9i52Pvd82Q-dwgLrzw-T2Xd1EPAZfTy7lDoaIu34M3ZCOG4DXsIc8cXgLfQ8kwAFXU4jpFl21kHXvznWOvl5fPldvZPOxfl8tN8RJKhKxxmjnoKqNYLZSqpasKrLt7LBmistCVbairaxFa5VlXGnKhXWgwIiCtZWYo4eTbvb4MzUxlTs_hSGfLJmU3FqjucoUOVEu-BhD05b5hR7CoWS0PAZY_gVYngPM_OOJ99P4D_oLztxyVQ</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1442997625</pqid></control><display><type>article</type><title>AD 775 pulse of cosmogenic radionuclides production as imprint of a Galactic gamma-ray burst</title><source>Oxford University Press Open Access</source><creator>Pavlov, A. K. ; Blinov, A. V. ; Konstantinov, A. N. ; Ostryakov, V. M. ; Vasilyev, G. I. ; Vdovina, M. A. ; Volkov, P. A.</creator><creatorcontrib>Pavlov, A. K. ; Blinov, A. V. ; Konstantinov, A. N. ; Ostryakov, V. M. ; Vasilyev, G. I. ; Vdovina, M. A. ; Volkov, P. A.</creatorcontrib><description>We suggest an explanation of a sharp increase in the abundance of cosmogenic radiocarbon found in tree rings dated AD 775. The increase could originate from high-energy irradiation of the atmosphere by a Galactic gamma-ray burst. We argue that, unlike a cosmic ray event, a gamma-ray burst does not necessarily result in a substantial increase in long-lived 10Be atmospheric production. At the same time, the 36Cl nuclide would be generated in the amounts detectable in the corresponding ice-core samples from Greenland and Antarctica. These peculiar features allow experimental discrimination of nuclide effects caused by gamma-ray bursts and by powerful proton events.</description><identifier>ISSN: 0035-8711</identifier><identifier>EISSN: 1365-2966</identifier><identifier>DOI: 10.1093/mnras/stt1468</identifier><language>eng</language><publisher>London: Oxford University Press</publisher><subject>Astrophysics ; Gamma ray astronomy ; Protons ; Star &amp; galaxy formation</subject><ispartof>Monthly notices of the Royal Astronomical Society, 2013-11, Vol.435 (4), p.2878-2884</ispartof><rights>2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society 2013</rights><rights>Copyright Oxford University Press, UK Nov 11, 2013</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c403t-9776ccabd7319b55d41b8966432d152485b9b0f4d3f95912560239ca5a7381fb3</citedby><cites>FETCH-LOGICAL-c403t-9776ccabd7319b55d41b8966432d152485b9b0f4d3f95912560239ca5a7381fb3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,1604,27924,27925</link.rule.ids><linktorsrc>$$Uhttps://dx.doi.org/10.1093/mnras/stt1468$$EView_record_in_Oxford_University_Press$$FView_record_in_$$GOxford_University_Press</linktorsrc></links><search><creatorcontrib>Pavlov, A. K.</creatorcontrib><creatorcontrib>Blinov, A. V.</creatorcontrib><creatorcontrib>Konstantinov, A. N.</creatorcontrib><creatorcontrib>Ostryakov, V. M.</creatorcontrib><creatorcontrib>Vasilyev, G. I.</creatorcontrib><creatorcontrib>Vdovina, M. A.</creatorcontrib><creatorcontrib>Volkov, P. A.</creatorcontrib><title>AD 775 pulse of cosmogenic radionuclides production as imprint of a Galactic gamma-ray burst</title><title>Monthly notices of the Royal Astronomical Society</title><addtitle>Mon. Not. R. Astron. Soc</addtitle><description>We suggest an explanation of a sharp increase in the abundance of cosmogenic radiocarbon found in tree rings dated AD 775. The increase could originate from high-energy irradiation of the atmosphere by a Galactic gamma-ray burst. We argue that, unlike a cosmic ray event, a gamma-ray burst does not necessarily result in a substantial increase in long-lived 10Be atmospheric production. At the same time, the 36Cl nuclide would be generated in the amounts detectable in the corresponding ice-core samples from Greenland and Antarctica. These peculiar features allow experimental discrimination of nuclide effects caused by gamma-ray bursts and by powerful proton events.</description><subject>Astrophysics</subject><subject>Gamma ray astronomy</subject><subject>Protons</subject><subject>Star &amp; galaxy formation</subject><issn>0035-8711</issn><issn>1365-2966</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2013</creationdate><recordtype>article</recordtype><recordid>eNqFkL1PwzAQxS0EEqUwsltiYTH1t-OxKlCQKrHAhhRdnKRK1cTBdob-97i0O9NJd7979-4hdM_oE6NWLPohQFzElJjUxQWaMaEV4VbrSzSjVChSGMau0U2MO0qpFFzP0PfyGRuj8DjtY4N9i52Pvd82Q-dwgLrzw-T2Xd1EPAZfTy7lDoaIu34M3ZCOG4DXsIc8cXgLfQ8kwAFXU4jpFl21kHXvznWOvl5fPldvZPOxfl8tN8RJKhKxxmjnoKqNYLZSqpasKrLt7LBmistCVbairaxFa5VlXGnKhXWgwIiCtZWYo4eTbvb4MzUxlTs_hSGfLJmU3FqjucoUOVEu-BhD05b5hR7CoWS0PAZY_gVYngPM_OOJ99P4D_oLztxyVQ</recordid><startdate>20131111</startdate><enddate>20131111</enddate><creator>Pavlov, A. K.</creator><creator>Blinov, A. V.</creator><creator>Konstantinov, A. N.</creator><creator>Ostryakov, V. M.</creator><creator>Vasilyev, G. I.</creator><creator>Vdovina, M. A.</creator><creator>Volkov, P. A.</creator><general>Oxford University Press</general><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>20131111</creationdate><title>AD 775 pulse of cosmogenic radionuclides production as imprint of a Galactic gamma-ray burst</title><author>Pavlov, A. K. ; Blinov, A. V. ; Konstantinov, A. N. ; Ostryakov, V. M. ; Vasilyev, G. I. ; Vdovina, M. A. ; Volkov, P. A.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c403t-9776ccabd7319b55d41b8966432d152485b9b0f4d3f95912560239ca5a7381fb3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2013</creationdate><topic>Astrophysics</topic><topic>Gamma ray astronomy</topic><topic>Protons</topic><topic>Star &amp; galaxy formation</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Pavlov, A. K.</creatorcontrib><creatorcontrib>Blinov, A. V.</creatorcontrib><creatorcontrib>Konstantinov, A. N.</creatorcontrib><creatorcontrib>Ostryakov, V. M.</creatorcontrib><creatorcontrib>Vasilyev, G. I.</creatorcontrib><creatorcontrib>Vdovina, M. A.</creatorcontrib><creatorcontrib>Volkov, P. A.</creatorcontrib><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Monthly notices of the Royal Astronomical Society</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Pavlov, A. K.</au><au>Blinov, A. V.</au><au>Konstantinov, A. N.</au><au>Ostryakov, V. M.</au><au>Vasilyev, G. I.</au><au>Vdovina, M. A.</au><au>Volkov, P. A.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>AD 775 pulse of cosmogenic radionuclides production as imprint of a Galactic gamma-ray burst</atitle><jtitle>Monthly notices of the Royal Astronomical Society</jtitle><stitle>Mon. Not. R. Astron. Soc</stitle><date>2013-11-11</date><risdate>2013</risdate><volume>435</volume><issue>4</issue><spage>2878</spage><epage>2884</epage><pages>2878-2884</pages><issn>0035-8711</issn><eissn>1365-2966</eissn><abstract>We suggest an explanation of a sharp increase in the abundance of cosmogenic radiocarbon found in tree rings dated AD 775. The increase could originate from high-energy irradiation of the atmosphere by a Galactic gamma-ray burst. We argue that, unlike a cosmic ray event, a gamma-ray burst does not necessarily result in a substantial increase in long-lived 10Be atmospheric production. At the same time, the 36Cl nuclide would be generated in the amounts detectable in the corresponding ice-core samples from Greenland and Antarctica. These peculiar features allow experimental discrimination of nuclide effects caused by gamma-ray bursts and by powerful proton events.</abstract><cop>London</cop><pub>Oxford University Press</pub><doi>10.1093/mnras/stt1468</doi><tpages>7</tpages><oa>free_for_read</oa></addata></record>
fulltext fulltext_linktorsrc
identifier ISSN: 0035-8711
ispartof Monthly notices of the Royal Astronomical Society, 2013-11, Vol.435 (4), p.2878-2884
issn 0035-8711
1365-2966
language eng
recordid cdi_proquest_journals_1442997625
source Oxford University Press Open Access
subjects Astrophysics
Gamma ray astronomy
Protons
Star & galaxy formation
title AD 775 pulse of cosmogenic radionuclides production as imprint of a Galactic gamma-ray burst
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-24T17%3A03%3A10IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_TOX&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=AD%20775%20pulse%20of%20cosmogenic%20radionuclides%20production%20as%20imprint%20of%20a%20Galactic%20gamma-ray%20burst&rft.jtitle=Monthly%20notices%20of%20the%20Royal%20Astronomical%20Society&rft.au=Pavlov,%20A.%20K.&rft.date=2013-11-11&rft.volume=435&rft.issue=4&rft.spage=2878&rft.epage=2884&rft.pages=2878-2884&rft.issn=0035-8711&rft.eissn=1365-2966&rft_id=info:doi/10.1093/mnras/stt1468&rft_dat=%3Cproquest_TOX%3E3103098901%3C/proquest_TOX%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c403t-9776ccabd7319b55d41b8966432d152485b9b0f4d3f95912560239ca5a7381fb3%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=1442997625&rft_id=info:pmid/&rft_oup_id=10.1093/mnras/stt1468&rfr_iscdi=true