FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2103177958> ?p ?o ?g. }

• W2103177958 abstract "Updated constraints on the dark matter cross section and mass are presented combining cosmic microwave background (CMB) power spectrum measurements from Planck, WMAP9, ACT, and SPT as well as several low-redshift data sets (BAO, HST, and supernovae). For the CMB data sets, we combine WMAP9 temperature and polarization data for $lensuremath{le}431$ with Planck temperature data for $432ensuremath{le}lensuremath{le}2500$, ACT and SPT data for $l>2500$, and Planck CMB four-point lensing measurements. We allow for redshift-dependent energy deposition from dark matter annihilation by using a ``universal energy absorption curve. We also include an updated treatment of the excitation, heating, and ionization energy fractions and provide an updated deposition efficiency factors (${f}_{text{eff}}$) for 41 different dark matter models. Assuming perfect energy deposition (${f}_{text{eff}}=1$) and a thermal cross section, dark matter masses below 26 GeV are excluded at the $2ensuremath{sigma}$ level. Assuming a more generic efficiency of ${f}_{text{eff}}=0.2$, thermal dark matter masses below 5 GeV are disfavored at the $2ensuremath{sigma}$ level. These limits are a factor of $ensuremath{sim}2$ improvement over those from WMAP9 data alone. These current constraints probe, but do not exclude, dark matter as an explanation for reported anomalous indirect detection observations from AMS-02/PAMELA and the Fermi gamma-ray inner-Galaxy data. They also probe relevant models that would explain anomalous direct detection events from CDMS, CRESST, CoGeNT, and DAMA, as originating from a generic thermal weakly interacting massive particle. Projected constraints from the full Planck release should improve the current limits by another factor of $ensuremath{sim}2$ but will not definitely probe these signals. The proposed CMB Stage IV experiment will more decisively explore the relevant regions and improve upon the Planck constraints by another factor of $ensuremath{sim}2$." @default.
• W2103177958 created "2016-06-24" @default.
• W2103177958 creator A5047206136 @default.
• W2103177958 creator A5055700518 @default.
• W2103177958 creator A5058817864 @default.
• W2103177958 date "2014-05-07" @default.
• W2103177958 modified "2023-10-18" @default.
• W2103177958 title "Current dark matter annihilation constraints from CMB and low-redshift data" @default.
• W2103177958 cites W1553693172 @default.
• W2103177958 cites W1859677373 @default.
• W2103177958 cites W1964742600 @default.
• W2103177958 cites W1968443673 @default.
• W2103177958 cites W1985999007 @default.
• W2103177958 cites W1988409168 @default.
• W2103177958 cites W1995962607 @default.
• W2103177958 cites W1997489115 @default.
• W2103177958 cites W2002002160 @default.
• W2103177958 cites W2019762720 @default.
• W2103177958 cites W2020972118 @default.
• W2103177958 cites W2022625885 @default.
• W2103177958 cites W2041676550 @default.
• W2103177958 cites W2042323747 @default.
• W2103177958 cites W2052306133 @default.
• W2103177958 cites W2067794112 @default.
• W2103177958 cites W2071587586 @default.
• W2103177958 cites W2074383387 @default.
• W2103177958 cites W2074628032 @default.
• W2103177958 cites W2078452600 @default.
• W2103177958 cites W2078775414 @default.
• W2103177958 cites W2090896155 @default.
• W2103177958 cites W2092587479 @default.
• W2103177958 cites W2098422406 @default.
• W2103177958 cites W2099025285 @default.
• W2103177958 cites W2108577214 @default.
• W2103177958 cites W2110370746 @default.
• W2103177958 cites W2110996783 @default.
• W2103177958 cites W2112456186 @default.
• W2103177958 cites W2113590725 @default.
• W2103177958 cites W2116312019 @default.
• W2103177958 cites W2120574945 @default.
• W2103177958 cites W2122765019 @default.
• W2103177958 cites W2126393358 @default.
• W2103177958 cites W2128476026 @default.
• W2103177958 cites W2133224752 @default.
• W2103177958 cites W2133952061 @default.
• W2103177958 cites W2138721573 @default.
• W2103177958 cites W2142290259 @default.
• W2103177958 cites W2142972164 @default.
• W2103177958 cites W2146049705 @default.
• W2103177958 cites W2148711716 @default.
• W2103177958 cites W2153208487 @default.
• W2103177958 cites W2156577128 @default.
• W2103177958 cites W2172214882 @default.
• W2103177958 cites W2594913691 @default.
• W2103177958 cites W3098540599 @default.
• W2103177958 cites W3099311733 @default.
• W2103177958 cites W3100537878 @default.
• W2103177958 cites W3101728852 @default.
• W2103177958 cites W3101954218 @default.
• W2103177958 cites W3105821254 @default.
• W2103177958 cites W3125978220 @default.
• W2103177958 doi "https://doi.org/10.1103/physrevd.89.103508" @default.
• W2103177958 hasPublicationYear "2014" @default.
• W2103177958 type Work @default.
• W2103177958 sameAs 2103177958 @default.
• W2103177958 citedByCount "141" @default.
• W2103177958 countsByYear W21031779582013 @default.
• W2103177958 countsByYear W21031779582014 @default.
• W2103177958 countsByYear W21031779582015 @default.
• W2103177958 countsByYear W21031779582016 @default.
• W2103177958 countsByYear W21031779582017 @default.
• W2103177958 countsByYear W21031779582018 @default.
• W2103177958 countsByYear W21031779582019 @default.
• W2103177958 countsByYear W21031779582020 @default.
• W2103177958 countsByYear W21031779582021 @default.
• W2103177958 countsByYear W21031779582022 @default.
• W2103177958 countsByYear W21031779582023 @default.
• W2103177958 crossrefType "journal-article" @default.
• W2103177958 hasAuthorship W2103177958A5047206136 @default.
• W2103177958 hasAuthorship W2103177958A5055700518 @default.
• W2103177958 hasAuthorship W2103177958A5058817864 @default.
• W2103177958 hasBestOaLocation W21031779582 @default.
• W2103177958 hasConcept C109214941 @default.
• W2103177958 hasConcept C121332964 @default.
• W2103177958 hasConcept C159249277 @default.
• W2103177958 hasConcept C166126730 @default.
• W2103177958 hasConcept C172790937 @default.
• W2103177958 hasConcept C201941533 @default.
• W2103177958 hasConcept C207297109 @default.
• W2103177958 hasConcept C26405456 @default.
• W2103177958 hasConcept C33024259 @default.
• W2103177958 hasConcept C44870925 @default.
• W2103177958 hasConcept C62520636 @default.
• W2103177958 hasConcept C66157390 @default.
• W2103177958 hasConcept C85725439 @default.
• W2103177958 hasConcept C98444146 @default.
• W2103177958 hasConceptScore W2103177958C109214941 @default.
• W2103177958 hasConceptScore W2103177958C121332964 @default.
• W2103177958 hasConceptScore W2103177958C159249277 @default.
• W2103177958 hasConceptScore W2103177958C166126730 @default.

• next