Correction: Beltrán, W. M. et al. Pentecostals, Gender Ideology and the Peace Plebiscite: Colombia 2016. Religions 9 (2018): 418

Beltrán, William Mauricio; Creely, Sian

doi:10.3390/rel10010060

Cited by 2 publications

(3 citation statements)

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“…Borehole strain-and tiltmeters can detect short-term elastic deformation transients from nearby SSEs at or below the earth's surface, which can be modeled to quantify the slip on the fault (e.g., Linde et al, 1996). The high spatial resolution (10s of m), global spatial coverage and precision (sub-cm over short distances) of synthetic aperture radarinterferometry (InSAR) (Bürgmann et al, 2000) is particularly well suited to image the distribution of shallow creep on faults around the world (e.g., Doubre and Peltzer, 2007, Jolivet et al, 2012, Thomas et al, 2014a, Turner et al, 2015Pousse Beltran et al, 2016).…”

Section: Geodetic Observationsmentioning

confidence: 99%

The geophysics, geology and mechanics of slow fault slip

Bürgmann

2018

Earth and Planetary Science Letters

322

308

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Modern geodetic and seismologic observations describe the behavior of fault slip over a vast range of spatial and temporal scales. Slip at sub-seismogenic speeds is evident from top to bottom of lithospheric faults and plays an important role throughout the earthquake cycle. Where earthquakes and tremor accompany slow slip, they help illuminate the spatiotemporal evolution of fault slip. Geophysical subsurface imaging and geologic field studies provide information about suitable environments of slow slip. In particular, exhumed fault and shear zones from various depths reveal the importance of multiple deformation processes and fault-zone structures. Most geologic examples feature frictionally weak and velocity-strengthening materials, well-developed mineral fabrics, and abundant veining indicative of near-lithostatic fluid pressure. To produce transient slow slip events and tremor, in addition to the presence of high-pressure fluids a heterogeneous fault-zone structure, composition, and/or metamorphic assemblage may be needed. Laboratory and computational models suggest that velocityweakening slip patches smaller than a critical dimension needed for earthquake nucleation will also fail in slow slip events. Changes in fluid pressure or slip ratecan cause a fault to transition between stable and unstable fault slip behavior. Future interdisciplinary investigations of slow fault slip, directly integrating geophysical, geological and modeling investigations, will further improve our understanding of the dynamics of slow slip and aid in providing more accurate earthquake hazard characterizations.

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Section: Geodetic Observationsmentioning

confidence: 99%

The geophysics, geology and mechanics of slow fault slip

Bürgmann

2018

Earth and Planetary Science Letters

322

308

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“…Below we will combine the above direct detection constraint with the LHC bounds for a scalar benchmark model. 6 In this study we use the LUX result as an example to illustrate the impact from direct detection experiments. As outlined in detail in the the LHC DM WG recommendation [5], also other experiments constrain this parameter space.…”

Section: Direct Detectionmentioning

confidence: 99%

“…Central to this effort are simplified DM models (SDMM), which have replaced interpretations using a universal set of operators in an effective field theory (EFT) [6][7][8][9][10][11] as the main vehicle to characterise DM searches at colliders. However, as discussed in [4], EFT interpretations can still provide useful information and complement the SDMM approach for collider searches.…”

Section: Introductionmentioning

confidence: 99%

Towards the next generation of simplified Dark Matter models

Albert

Bauer

Brooke

et al. 2017

Physics of the Dark Universe

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Abstract:This White Paper is an input to the ongoing discussion about the extension and refinement of simplified Dark Matter (DM) models. Based on two concrete examples, we show how existing simplified DM models (SDMM) can be extended to provide a more accurate and comprehensive framework to interpret and characterise collider searches. In the first example we extend the canonical SDMM with a scalar mediator to include mixing with the Higgs boson. We show that this approach not only provides a better description of the underlying kinematic properties that a complete model would possess, but also offers the option of using this more realistic class of scalar mixing models to compare and combine consistently searches based on different experimental signatures. The second example outlines how a new physics signal observed in a visible channel can be connected to DM by extending a simplified model including effective couplings. This discovery scenario uses the recently observed excess in the high-mass diphoton searches of ATLAS and CMS for a case study to show that such a pragmatic approach can aid the experimental search programme to verify/falsify a potential signal and to study its underlying nature. In the next part of the White Paper we outline other interesting options for SDMM that could be studied in more detail in the future. Finally, we discuss important aspects of supersymmetric models for DM and how these could help to develop of more complete SDMM.This White Paper is a summary of the brainstorming meeting "Next generation of simplified Dark Matter models" that took place at Imperial College, London on May 6, 2016, and corresponding follow-up studies on selected subjects.

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Correction: Beltrán, W. M. et al. Pentecostals, Gender Ideology and the Peace Plebiscite: Colombia 2016. Religions 9 (2018): 418

Abstract: The authors wish to make the following corrections to (Beltrán and Creely 2018) [...]

Cited by 2 publications

References 1 publication

The geophysics, geology and mechanics of slow fault slip

The geophysics, geology and mechanics of slow fault slip

Towards the next generation of simplified Dark Matter models

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