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author | Bryan Newbold <bnewbold@robocracy.org> | 2019-03-05 17:35:36 -0800 |
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committer | Bryan Newbold <bnewbold@robocracy.org> | 2019-05-21 11:41:29 -0700 |
commit | 3ec275c7d78aa261027f35c26366a382c5dd7a6c (patch) | |
tree | 9356ac9a145a4709c0a8339eb751f4c4d7840936 /python/tests/files/arxivraw_1810.09584.xml | |
parent | 6fc6232250241b3bfdddb5e62501a26dfaac6827 (diff) | |
download | fatcat-3ec275c7d78aa261027f35c26366a382c5dd7a6c.tar.gz fatcat-3ec275c7d78aa261027f35c26366a382c5dd7a6c.zip |
basic arxivraw XML parser
Diffstat (limited to 'python/tests/files/arxivraw_1810.09584.xml')
-rw-r--r-- | python/tests/files/arxivraw_1810.09584.xml | 31 |
1 files changed, 31 insertions, 0 deletions
diff --git a/python/tests/files/arxivraw_1810.09584.xml b/python/tests/files/arxivraw_1810.09584.xml new file mode 100644 index 00000000..55ce381f --- /dev/null +++ b/python/tests/files/arxivraw_1810.09584.xml @@ -0,0 +1,31 @@ +<?xml version="1.0" encoding="UTF-8"?> +<OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd"> +<responseDate>2019-03-05T23:10:23Z</responseDate> +<request verb="GetRecord" identifier="oai:arXiv.org:1810.09584" metadataPrefix="arXivRaw">http://export.arxiv.org/oai2</request> +<GetRecord> +<record> +<header> + <identifier>oai:arXiv.org:1810.09584</identifier> + <datestamp>2019-01-15</datestamp> + <setSpec>physics:cond-mat</setSpec> + <setSpec>physics:physics</setSpec> +</header> +<metadata> + <arXivRaw xmlns="http://arxiv.org/OAI/arXivRaw/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://arxiv.org/OAI/arXivRaw/ http://arxiv.org/OAI/arXivRaw.xsd"> + <id>1810.09584</id><submitter>\'Edgar Rold\'an</submitter><version version="v1"><date>Mon, 22 Oct 2018 22:41:50 GMT</date><size>401kb</size><source_type>D</source_type></version><version version="v2"><date>Sun, 13 Jan 2019 11:17:09 GMT</date><size>669kb</size><source_type>D</source_type></version><title>Martingale theory for housekeeping heat</title><authors>Raphael Chetrite, Shamik Gupta, Izaak Neri and \'Edgar Rold\'an</authors><categories>cond-mat.stat-mech physics.bio-ph physics.data-an</categories><comments>7 pages, 2 figures</comments><journal-ref>EPL 124,60006 (2018)</journal-ref><doi>10.1209/0295-5075/124/60006</doi><license>http://arxiv.org/licenses/nonexclusive-distrib/1.0/</license><abstract> The housekeeping heat is the energy exchanged between a system and its +environment in a nonequilibrium process that results from the violation of +detailed balance. We describe fluctuations of the housekeeping heat in +mesoscopic systems using the theory of martingales, a mathematical framework +widely used in probability theory and finance. We show that the exponentiated +housekeeping heat (in units of $k_{\rm B}T$, with $k_{\rm B}$ the Boltzmann +constant and $T$ the temperature) of a Markovian nonequilibrium process under +arbitrary time-dependent driving is a martingale process. From this result, we +derive universal equalities and inequalities for the statistics of +stopping-times and suprema of the housekeeping heat. We test our results with +numerical simulations of a system driven out of equilibrium and described by +Langevin dynamics. +</abstract></arXivRaw> +</metadata> +</record> +</GetRecord> +</OAI-PMH> |