Search results for "QB"

showing 10 items of 522 documents

Dust Production and Particle Acceleration in Supernova 1987A Revealed with ALMA

2013

Supernova (SN) explosions are crucial engines driving the evolution of galaxies by shock heating gas, increasing the metallicity, creating dust, and accelerating energetic particles. In 2012 we used the Atacama Large Millimeter/Submillimeter Array to observe SN 1987A, one of the best-observed supernovae since the invention of the telescope. We present spatially resolved images at 450um, 870um, 1.4mm, and 2.8mm, an important transition wavelength range. Longer wavelength emission is dominated by synchrotron radiation from shock-accelerated particles, shorter wavelengths by emission from the largest mass of dust measured in a supernova remnant (>0.2Msun). For the first time we show unambig…

MetallicityAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesSynchrotron radiationAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsSubmillimeter ArrayEARLY UNIVERSEindividual (1987A) [supernovae]Magellanic CloudsAstrophysics::Solar and Stellar AstrophysicsEjectaSupernova remnantSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsQBHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsISM [galaxies]supernova remnants [ISM]Astronomy and AstrophysicsOPTICAL-PROPERTIESHUBBLE-SPACE-TELESCOPEAstrophysics - Astrophysics of GalaxiesEVOLUTIONGalaxyParticle accelerationEJECTASupernovaPhysics and AstronomyAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)REVERSE SHOCKREMNANTAstrophysics::Earth and Planetary AstrophysicsEMISSIONAstrophysics - High Energy Astrophysical PhenomenaMASSIVE STARSSN 1987A
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Comparison of high‐speed optical observations of a lightning flash from space and the ground

2020

We analyze a nighttime negative cloud-to-ground lightning flash in Colombia observed from the ground with a high-speed camera at 5,000 images per second and from space by the Atmosphere-Space Interactions Monitor (ASIM) on the International Space Station (ISS), the Lightning Imaging Sensor also on the ISS (ISS-LIS), and the Geostationary Lightning Mapper (GLM) on GOES-16. The space instruments measure the oxygen band at 777.4 nm, allowing for direct comparisons of measurements, and the ground-based camera observes in a wide visible band. After conversion to energy emitted at the cloud top, we find a good linear correspondence of the optical energies measured by the three space instruments, …

MeteorologyGeostationary lightning mapperlcsh:AstronomyEnvironmental Science (miscellaneous)Space (mathematics):Enginyeria dels materials [Àrees temàtiques de la UPC]Lightningatmosphere‐space interactions monitorlightning imaging sensorlcsh:QB1-991Flash (photography)geostationary lightning mappercloudthunderstormAtmosphere-space interactions monitorlcsh:QE1-996.5Lightninglcsh:GeologyThunderstormThunderstormGeneral Earth and Planetary SciencesEnvironmental scienceLightning imaging sensorlightningCloudLlamps
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Multivariate and Multiscale Complexity of Long-Range Correlated Cardiovascular and Respiratory Variability Series

2020

Assessing the dynamical complexity of biological time series represents an important topic with potential applications ranging from the characterization of physiological states and pathological conditions to the calculation of diagnostic parameters. In particular, cardiovascular time series exhibit a variability produced by different physiological control mechanisms coupled with each other, which take into account several variables and operate across multiple time scales that result in the coexistence of short term dynamics and long-range correlations. The most widely employed technique to evaluate the dynamical complexity of a time series at different time scales, the so-called multiscale …

Multivariate statisticsSystolic arterial pressure (SAP)Vector autoregressive fractionally integrated (VARFI) modelsComputer scienceGeneral Physics and Astronomylcsh:Astrophysics01 natural sciencesArticle010305 fluids & plasmaslcsh:QB460-4660103 physical sciencesRange (statistics)Multi-scale entropy (MSE)lcsh:Science010306 general physicsRepresentation (mathematics)Parametric statisticsvector autoregressive fractionally integrated (VARFI) modelSeries (mathematics)multi-scale entropy (MSE)Stochastic processsystolic arterial pressure (SAP)lcsh:QC1-999Term (time)Autoregressive modelSettore ING-INF/06 - Bioingegneria Elettronica E Informaticavector autoregressive fractionally integrated (VARFI) modelslcsh:QBiological systemHeart rate variability (HRV)lcsh:Physicsheart rate variability (HRV)
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"Table 1" of "t anti-t production cross-section in p anti-p collisions at s**(1/2) = 1.8-TeV"

2002

Measured top quark pair production cross section in the different channels and the various averages, including the overall average.

Nonlinear Sciences::Exactly Solvable and Integrable Systems1800.0High Energy Physics::LatticeHigh Energy Physics::PhenomenologyIntegrated Cross SectionPhysics::Atomic and Molecular ClustersExclusive1.727E+061.727E+06Cross SectionSIGPBAR P --> TQ TQBAR
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What is the final state of a black hole merger?

2018

In this short paper we discuss the possibility of testing the nature of astrophysical black holes using the recently observed black hole mergers. We investigate the possibility that a secondary black hole is created in the merger of two astrophysical black holes and discuss potential astrophysical signatures. We point out that black hole mergers are a possible astrophysical mechanism for the creation of quantum black holes with masses close to the Planck mass.

Nuclear and High Energy PhysicsBlack holeAstrophysics::High Energy Astrophysical PhenomenaShort paperPlanck massFOS: Physical sciencesGeneral Physics and AstronomyGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum Cosmology0103 physical sciencesquantum black holes.10. No inequality010306 general physicsQuantumQBPhysics010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsBlack holeblack hole mergerquantum gravityQuantum gravityModern Physics Letters A
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"Table 5" of "Measurement of the $t\bar{t}Z$ and $t\bar{t}W$ cross sections in proton-proton collisions at $\sqrt{s}=13$ TeV with the ATLAS detector"

2019

The expected and observed 68% and 95% confidence intervals, which include the value 0, for $\mathcal{C}_{i}/\Lambda^{2}$ for the EFT coefficients $\mathcal{C}_{\phi Q}^{(3)}$, $\mathcal{C}_{\phi t}$, $\mathcal{C}_{tB}$ and $\mathcal{C}_{tW}$. The intervals for $\mathcal{C}_{\phi Q}^{(3)}$ are derived setting $\mathcal{C}_{\phi Q}^{(1)}$ to zero; the measurement is sensitive to the difference $\mathcal{C}_{\phi Q}^{(3)}-\mathcal{C}_{\phi Q}^{(1)}$. All results are given in units of 1/TeV$^{2}$. Limits from fits for the EFT coefficients with only the linear term are also shown.

P P --> TQ TQBAR Z0 XP P --> TQ TQBAR W+ XProton-Proton ScatteringCLStop physicsP P --> TQ TQBAR W- Xflavor physicsCross SectionEFT coefficients bounds13000
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"Table 2" of "Measurement of the $t\bar{t}Z$ and $t\bar{t}W$ cross sections in proton-proton collisions at $\sqrt{s}=13$ TeV with the ATLAS detector"

2019

68% confidence level (CL) contours of the measured $t\bar{t}Z$ and $t\bar{t}W$ cross sections.

P P --> TQ TQBAR Z0 XP P --> TQ TQBAR W+ XProton-Proton ScatteringCLStop physicsP P --> TQ TQBAR W- Xflavor physicsCross SectionSIG13000
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"Table 3" of "Measurement of the $t\bar{t}Z$ and $t\bar{t}W$ cross sections in proton-proton collisions at $\sqrt{s}=13$ TeV with the ATLAS detector"

2019

95% confidence level (CL) contours of the measured $t\bar{t}Z$ and $t\bar{t}W$ cross sections.

P P --> TQ TQBAR Z0 XP P --> TQ TQBAR W+ XProton-Proton ScatteringCLStop physicsP P --> TQ TQBAR W- Xflavor physicsCross SectionSIG13000
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"Table 1" of "Measurement of the $t\bar{t}Z$ and $t\bar{t}W$ cross sections in proton-proton collisions at $\sqrt{s}=13$ TeV with the ATLAS detector"

2019

The result of the simultaneous fit to the $t\bar{t}Z$ and $t\bar{t}W$ cross sections.

P P --> TQ TQBAR Z0 XP P --> TQ TQBAR W+ XProton-Proton Scatteringtop physicsHigh Energy Physics::PhenomenologyP P --> TQ TQBAR W- Xflavor physicsHigh Energy Physics::ExperimentCross SectionSIG13000
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"Table 4" of "Measurement of the $t\bar{t}Z$ and $t\bar{t}W$ cross sections in proton-proton collisions at $\sqrt{s}=13$ TeV with the ATLAS detector"

2019

List of relative uncertainties in the measured cross sections of the $t\bar{t}Z$ and $t\bar{t}W$ processes from the fit, grouped in categories. All uncertainties are symmetrized. The sum in quadrature may not be equal to the total due to correlations between uncertainties introduced by the fit.

P P --> TQ TQBAR Z0 XP P --> TQ TQBAR W+ XProton-Proton Scatteringtop physicsP P --> TQ TQBAR W- Xflavor physicsCross SectionSIG13000
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