PArthENoPE Revolutions
This paper presents the main features of a new and updated version of the program PArthENoPE, which the community has been using for many years for computing the abundances of light elements produced during Big Bang Nucleosynthesis. This is the third release of the PArthENoPE code, after the 2008 an...
Gespeichert in:
Veröffentlicht in: | arXiv.org 2021-03 |
---|---|
Hauptverfasser: | , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | |
---|---|
container_issue | |
container_start_page | |
container_title | arXiv.org |
container_volume | |
creator | Gariazzo, S de Salas, P F Pisanti, O Consiglio, R |
description | This paper presents the main features of a new and updated version of the program PArthENoPE, which the community has been using for many years for computing the abundances of light elements produced during Big Bang Nucleosynthesis. This is the third release of the PArthENoPE code, after the 2008 and the 2018 ones, and will be distributed from the code's website, http://parthenope.na.infn.it. Apart from minor changes, the main improvements in this new version include a revisited implementation of the nuclear rates for the most important reactions of deuterium destruction, H2(p,gamma)He3, H2(d, n)He3 and H2(d, p)H3, and a re-designed GUI, which extends the functionality of the previous one. The new GUI, in particular, supersedes the previous tools for running over grids of parameters with a better management of parallel runs, and it offers a brand-new set of functions for plotting the results. |
doi_str_mv | 10.48550/arxiv.2103.05027 |
format | Article |
fullrecord | <record><control><sourceid>proquest_arxiv</sourceid><recordid>TN_cdi_arxiv_primary_2103_05027</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2499692689</sourcerecordid><originalsourceid>FETCH-LOGICAL-a529-993f326445be1d71336d50e9e06f830763823963ff2613461a3dc1a2fd738d463</originalsourceid><addsrcrecordid>eNotzkFLAzEQhuEgCJbaq-BJwfOuk5lkNjmWslqhaJHeQzQJbqndmt0t-u-trafv8vLxCHEtoVRGa7j3-bvZlyiBStCA1ZkYIZEsjEK8EJOuWwMAcoVa00hcLae5_6if22V9-xr37Wbom3bbXYrz5DddnPzvWKwe6tVsXixeHp9m00XhNdrCWkqErJR-izJUkoiDhmgjcDIEFZNBskwpIUtSLD2Fd-kxhYpMUExjcXO6PaLdLjefPv-4P7w74g_F3anY5fZriF3v1u2QtweTQ2UtW2Rj6RfQLkN-</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2499692689</pqid></control><display><type>article</type><title>PArthENoPE Revolutions</title><source>arXiv.org</source><source>Free E- Journals</source><creator>Gariazzo, S ; de Salas, P F ; Pisanti, O ; Consiglio, R</creator><creatorcontrib>Gariazzo, S ; de Salas, P F ; Pisanti, O ; Consiglio, R</creatorcontrib><description>This paper presents the main features of a new and updated version of the program PArthENoPE, which the community has been using for many years for computing the abundances of light elements produced during Big Bang Nucleosynthesis. This is the third release of the PArthENoPE code, after the 2008 and the 2018 ones, and will be distributed from the code's website, http://parthenope.na.infn.it. Apart from minor changes, the main improvements in this new version include a revisited implementation of the nuclear rates for the most important reactions of deuterium destruction, H2(p,gamma)He3, H2(d, n)He3 and H2(d, p)H3, and a re-designed GUI, which extends the functionality of the previous one. The new GUI, in particular, supersedes the previous tools for running over grids of parameters with a better management of parallel runs, and it offers a brand-new set of functions for plotting the results.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.2103.05027</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Big bang cosmology ; Deuterium ; Graphical user interface ; Light elements ; Nuclear fusion ; Nuclei (nuclear physics) ; Physics - Instrumentation and Methods for Astrophysics ; Websites</subject><ispartof>arXiv.org, 2021-03</ispartof><rights>2021. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,780,784,885,27925</link.rule.ids><backlink>$$Uhttps://doi.org/10.48550/arXiv.2103.05027$$DView paper in arXiv$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.1016/j.cpc.2021.108205$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink></links><search><creatorcontrib>Gariazzo, S</creatorcontrib><creatorcontrib>de Salas, P F</creatorcontrib><creatorcontrib>Pisanti, O</creatorcontrib><creatorcontrib>Consiglio, R</creatorcontrib><title>PArthENoPE Revolutions</title><title>arXiv.org</title><description>This paper presents the main features of a new and updated version of the program PArthENoPE, which the community has been using for many years for computing the abundances of light elements produced during Big Bang Nucleosynthesis. This is the third release of the PArthENoPE code, after the 2008 and the 2018 ones, and will be distributed from the code's website, http://parthenope.na.infn.it. Apart from minor changes, the main improvements in this new version include a revisited implementation of the nuclear rates for the most important reactions of deuterium destruction, H2(p,gamma)He3, H2(d, n)He3 and H2(d, p)H3, and a re-designed GUI, which extends the functionality of the previous one. The new GUI, in particular, supersedes the previous tools for running over grids of parameters with a better management of parallel runs, and it offers a brand-new set of functions for plotting the results.</description><subject>Big bang cosmology</subject><subject>Deuterium</subject><subject>Graphical user interface</subject><subject>Light elements</subject><subject>Nuclear fusion</subject><subject>Nuclei (nuclear physics)</subject><subject>Physics - Instrumentation and Methods for Astrophysics</subject><subject>Websites</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2021</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GOX</sourceid><recordid>eNotzkFLAzEQhuEgCJbaq-BJwfOuk5lkNjmWslqhaJHeQzQJbqndmt0t-u-trafv8vLxCHEtoVRGa7j3-bvZlyiBStCA1ZkYIZEsjEK8EJOuWwMAcoVa00hcLae5_6if22V9-xr37Wbom3bbXYrz5DddnPzvWKwe6tVsXixeHp9m00XhNdrCWkqErJR-izJUkoiDhmgjcDIEFZNBskwpIUtSLD2Fd-kxhYpMUExjcXO6PaLdLjefPv-4P7w74g_F3anY5fZriF3v1u2QtweTQ2UtW2Rj6RfQLkN-</recordid><startdate>20210308</startdate><enddate>20210308</enddate><creator>Gariazzo, S</creator><creator>de Salas, P F</creator><creator>Pisanti, O</creator><creator>Consiglio, R</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope><scope>GOX</scope></search><sort><creationdate>20210308</creationdate><title>PArthENoPE Revolutions</title><author>Gariazzo, S ; de Salas, P F ; Pisanti, O ; Consiglio, R</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a529-993f326445be1d71336d50e9e06f830763823963ff2613461a3dc1a2fd738d463</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2021</creationdate><topic>Big bang cosmology</topic><topic>Deuterium</topic><topic>Graphical user interface</topic><topic>Light elements</topic><topic>Nuclear fusion</topic><topic>Nuclei (nuclear physics)</topic><topic>Physics - Instrumentation and Methods for Astrophysics</topic><topic>Websites</topic><toplevel>online_resources</toplevel><creatorcontrib>Gariazzo, S</creatorcontrib><creatorcontrib>de Salas, P F</creatorcontrib><creatorcontrib>Pisanti, O</creatorcontrib><creatorcontrib>Consiglio, R</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection><collection>arXiv.org</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Gariazzo, S</au><au>de Salas, P F</au><au>Pisanti, O</au><au>Consiglio, R</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>PArthENoPE Revolutions</atitle><jtitle>arXiv.org</jtitle><date>2021-03-08</date><risdate>2021</risdate><eissn>2331-8422</eissn><abstract>This paper presents the main features of a new and updated version of the program PArthENoPE, which the community has been using for many years for computing the abundances of light elements produced during Big Bang Nucleosynthesis. This is the third release of the PArthENoPE code, after the 2008 and the 2018 ones, and will be distributed from the code's website, http://parthenope.na.infn.it. Apart from minor changes, the main improvements in this new version include a revisited implementation of the nuclear rates for the most important reactions of deuterium destruction, H2(p,gamma)He3, H2(d, n)He3 and H2(d, p)H3, and a re-designed GUI, which extends the functionality of the previous one. The new GUI, in particular, supersedes the previous tools for running over grids of parameters with a better management of parallel runs, and it offers a brand-new set of functions for plotting the results.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.2103.05027</doi><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | EISSN: 2331-8422 |
ispartof | arXiv.org, 2021-03 |
issn | 2331-8422 |
language | eng |
recordid | cdi_arxiv_primary_2103_05027 |
source | arXiv.org; Free E- Journals |
subjects | Big bang cosmology Deuterium Graphical user interface Light elements Nuclear fusion Nuclei (nuclear physics) Physics - Instrumentation and Methods for Astrophysics Websites |
title | PArthENoPE Revolutions |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-07T09%3A29%3A42IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_arxiv&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=PArthENoPE%20Revolutions&rft.jtitle=arXiv.org&rft.au=Gariazzo,%20S&rft.date=2021-03-08&rft.eissn=2331-8422&rft_id=info:doi/10.48550/arxiv.2103.05027&rft_dat=%3Cproquest_arxiv%3E2499692689%3C/proquest_arxiv%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2499692689&rft_id=info:pmid/&rfr_iscdi=true |