<?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>2017-12-14T13:00:41Z</responseDate>
<request verb="ListRecords" from="2017-12-14" metadataPrefix="arXiv" set="physics:hep-ex">http://export.arxiv.org/oai2</request>
<ListRecords>
<record>
<header>
 <identifier>oai:arXiv.org:1706.05371</identifier>
 <datestamp>2017-12-14</datestamp>
 <setSpec>physics:hep-ex</setSpec>
</header>
<metadata>
 <arXiv xmlns="http://arxiv.org/OAI/arXiv/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://arxiv.org/OAI/arXiv/ http://arxiv.org/OAI/arXiv.xsd">
 <id>1706.05371</id><created>2017-06-16</created><updated>2017-12-12</updated><authors><author><keyname>Anderson</keyname><forenames>Tyler</forenames></author><author><keyname>Cutter</keyname><forenames>Jacob</forenames></author><author><keyname>Dhaliwal</keyname><forenames>Navneet</forenames></author><author><keyname>Dalager</keyname><forenames>Olivia</forenames></author><author><keyname>Godfrey</keyname><forenames>Benjamin</forenames></author><author><keyname>Hillbrand</keyname><forenames>Seth</forenames></author><author><keyname>Irving</keyname><forenames>Michael</forenames></author><author><keyname>Manalaysay</keyname><forenames>Aaron</forenames></author><author><keyname>Montoya</keyname><forenames>Juan</forenames></author><author><keyname>Morad</keyname><forenames>James</forenames></author><author><keyname>Neher</keyname><forenames>Christian</forenames></author><author><keyname>Stolp</keyname><forenames>Dustin</forenames></author><author><keyname>Tripathi</keyname><forenames>Mani</forenames></author></authors><title>Evaluation of Silicon Photomultipliers for use as Photosensors in Liquid
  Xenon Detectors</title><categories>physics.ins-det hep-ex</categories><comments>10 pages, 9 figures</comments><license>http://arxiv.org/licenses/nonexclusive-distrib/1.0/</license><abstract>  Silicon photomultipliers (SiPMs) are potential solid-state alternatives to
traditional photomultiplier tubes (PMTs) for single-photon detection. In this
paper, we report on evaluating SensL MicroFC-10035-SMT SiPMs for their
suitability as PMT replacements. The devices were successfully operated in a
liquid-xenon detector, which demonstrates that SiPMs can be used in noble
element time projection chambers as photosensors. The devices were also cooled
down to 170 K to observe dark count dependence on temperature. No dependencies
on the direction of an applied 3.2 kV/cm electric field were observed with
respect to dark-count rate, gain, or photon detection efficiency.
</abstract></arXiv>
</metadata>
</record>
<record>
<header>
 <identifier>oai:arXiv.org:1706.09418</identifier>
 <datestamp>2017-12-14</datestamp>
 <setSpec>physics:hep-ex</setSpec>
</header>
<metadata>
 <arXiv xmlns="http://arxiv.org/OAI/arXiv/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://arxiv.org/OAI/arXiv/ http://arxiv.org/OAI/arXiv.xsd">
 <id>1706.09418</id><created>2017-06-28</created><updated>2017-11-26</updated><authors><author><keyname>Dercks</keyname><forenames>Daniel</forenames></author><author><keyname>Dreiner</keyname><forenames>Herbi</forenames></author><author><keyname>Krauss</keyname><forenames>Manuel E.</forenames></author><author><keyname>Opferkuch</keyname><forenames>Toby</forenames></author><author><keyname>Reinert</keyname><forenames>Annika</forenames></author></authors><title>R-Parity Violation at the LHC</title><categories>hep-ph hep-ex</categories><comments>43 pages, 13 tables, 17 figures; updated Figs. 11-17 and Tab. 12
  including NLO corrections; version accepted for publication in EPJC</comments><report-no>BONN-TH-2017-03</report-no><journal-ref>Eur. Phys. J. C (2017) 77:856</journal-ref><doi>10.1140/epjc/s10052-017-5414-4</doi><license>http://arxiv.org/licenses/nonexclusive-distrib/1.0/</license><abstract>  We investigate the phenomenology of the MSSM extended by a single R-parity
violating coupling at the unification scale. For all R-parity violating
couplings, we discuss the evolution of the particle spectra through the
renormalization group equations and the nature of the lightest supersymmetric
particle (LSP) within the CMSSM, as an example of a specific complete
supersymmetric model. We use the nature of the LSP to classify the possible
signatures. For each possible scenario we present in detail the current LHC
bounds on the supersymmetric particle masses, typically obtained using
simplified models. From this we determine the present coverage of R-parity
violating models at the LHC. We find several gaps, in particular for a
stau-LSP, which is easily obtained in R-parity violating models. Using the
program CheckMATE we recast existing LHC searches to set limits on the
parameters of all R-parity violating CMSSMs. We find that virtually all of them
are either more strongly constrained or similarly constrained in comparison to
the R-parity conserving CMSSM, including the $\bar U\bar D\bar D$ models. For
each R-parity violating CMSSM we then give the explicit lower mass bounds on
all relevant supersymmetric particles.
</abstract></arXiv>
</metadata>
</record>
<record>
<header>
 <identifier>oai:arXiv.org:1707.00874</identifier>
 <datestamp>2017-12-14</datestamp>
 <setSpec>physics:hep-ex</setSpec>
</header>
<metadata>
 <arXiv xmlns="http://arxiv.org/OAI/arXiv/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://arxiv.org/OAI/arXiv/ http://arxiv.org/OAI/arXiv.xsd">
 <id>1707.00874</id><created>2017-07-04</created><updated>2017-12-13</updated><authors><author><keyname>Bandyopadhyay</keyname><forenames>Priyotosh</forenames></author><author><keyname>Chun</keyname><forenames>Eung Jin</forenames></author><author><keyname>Mandal</keyname><forenames>Rusa</forenames></author></authors><title>Implications of right-handed neutrinos in $B-L$ extended standard model
  with scalar dark matter</title><categories>hep-ph astro-ph.CO hep-ex</categories><comments>Typos corrected, references added, version accepted for publication
  in PRD</comments><report-no>IITH-PH-0001/17, IMSc/2017/07/05</report-no><license>http://arxiv.org/licenses/nonexclusive-distrib/1.0/</license><abstract>  We investigate the Standard Model (SM) with a $U(1)_{B-L}$ gauge extension
where a $B-L$ charged scalar is a viable dark matter (DM) candidate. The
dominant annihilation process, for the DM particle is through the $B-L$
symmetry breaking scalar to right-handed neutrino pair. We exploit the effect
of decay and inverse decay of the right-handed neutrino in thermal relic
abundance of the DM. Depending on the values of the decay rate, the DM relic
density can be significantly different from what is obtained in the standard
calculation assuming the right-handed neutrino is in thermal equilibrium and
there appear different regions of the parameter space satisfying the observed
DM relic density. For a DM mass less than $\mathcal{O}$(TeV), the direct
detection experiments impose a competitive bound on the mass of the
$U(1)_{B-L}$ gauge boson $Z^\prime$ with the collider experiments. Utilizing
the non-observation of the displaced vertices arising from the right-handed
neutrino decays, bound on the mass of $Z^\prime$ has been obtained at present
and higher luminosities at the LHC with 14 TeV centre of mass energy where an
integrated luminosity of 100fb$^{-1}$ is sufficient to probe $m_{Z'} \sim 5.5$
TeV.
</abstract></arXiv>
</metadata>
</record>
</ListRecords>
</OAI-PMH>
