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Particle Acceleration At Astrophysical Shocks PowerPoint PPT Presentation
Particle Acceleration At Astrophysical Shocks - Title: Slide 1 Last modified by: SCIPP Document presentation format: Custom Other titles: Times New Roman Tahoma Arial Wingdings Avant Garde Gothic Comic Sans MS ...
Title: Slide 1 Last modified by: SCIPP Document presentation format: Custom Other titles: Times New Roman Tahoma Arial Wingdings Avant Garde Gothic Comic Sans MS ...
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Hot Cold Molecules: Collisions at Astrophysical Temperatures PowerPoint PPT Presentation
Hot Cold Molecules: Collisions at Astrophysical Temperatures - Hot Cold Molecules: Collisions at Astrophysical Temperatures Frank C. De Lucia Ohio State University * * * * * * * * * * * * * * * * * * Atom Envy, Molecule Envy ...
Hot Cold Molecules: Collisions at Astrophysical Temperatures Frank C. De Lucia Ohio State University * * * * * * * * * * * * * * * * * * Atom Envy, Molecule Envy ...
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Spectral modeling and diagnostics in various astrophysical environments PowerPoint PPT Presentation
Spectral modeling and diagnostics in various astrophysical environments - Spectral modeling and diagnostics in various astrophysical environments Jelle Kaastra SRON Topics Multi-temperature structure Resonance scattering in groups of ...
Spectral modeling and diagnostics in various astrophysical environments Jelle Kaastra SRON Topics Multi-temperature structure Resonance scattering in groups of ...
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Introduction to Astrophysical Gas Dynamics PowerPoint PPT Presentation
Introduction to Astrophysical Gas Dynamics - Vorticity: swirling motions within a flow as. a dynamical entity: long-lived structures ... Interpretation of the vorticity equation. Vortex. stretching ...
Vorticity: swirling motions within a flow as. a dynamical entity: long-lived structures ... Interpretation of the vorticity equation. Vortex. stretching ...
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The Future: Astrophysical and Cosmological Data PowerPoint PPT Presentation
The Future: Astrophysical and Cosmological Data - The Future: Astrophysical and Cosmological Data
The Future: Astrophysical and Cosmological Data
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Introduction to Astrophysical Gas Dynamics PowerPoint PPT Presentation
Introduction to Astrophysical Gas Dynamics - a dynamical entity: long-lived structures. due to Kelvin's ... Global Eastward Circulation! More extreme example: Jupiter's cloud bands. Great Red Spot ...
a dynamical entity: long-lived structures. due to Kelvin's ... Global Eastward Circulation! More extreme example: Jupiter's cloud bands. Great Red Spot ...
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General Astrophysical Concepts: Astronomical length scales and time scales PowerPoint PPT Presentation
General Astrophysical Concepts: Astronomical length scales and time scales - Cosmic Microwave Background Radiation (after-glow from the ... Homogeneity implies isotropy, But isotropy does NOT imply homogeneity. Kepler's laws of motion ...
Cosmic Microwave Background Radiation (after-glow from the ... Homogeneity implies isotropy, But isotropy does NOT imply homogeneity. Kepler's laws of motion ...
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Astrophysical Sources of Stochastic Gravitational-Wave Background PowerPoint PPT Presentation
Astrophysical Sources of Stochastic Gravitational-Wave Background - ... statistic (Drasco et al. 2003), Probability Event Horizon (Coward et al. 2005) ... Neutron star formation: Blair & Ju 1996, Coward et al. 2001-02, Howell et al. ...
... statistic (Drasco et al. 2003), Probability Event Horizon (Coward et al. 2005) ... Neutron star formation: Blair & Ju 1996, Coward et al. 2001-02, Howell et al. ...
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The German Astrophysical Virtual Observatory (GAVO) PowerPoint PPT Presentation
The German Astrophysical Virtual Observatory (GAVO) - Grid computing: simulations, distributed cluster finder ... Largest cosmological simulation to date. 10 billion particles evolving under gravity ...
Grid computing: simulations, distributed cluster finder ... Largest cosmological simulation to date. 10 billion particles evolving under gravity ...
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General Astrophysical Concepts: Astronomical length scales and time scales PowerPoint PPT Presentation
General Astrophysical Concepts: Astronomical length scales and time scales - Title: General Astrophysical Concepts: Astronomical length scales and time scales Author: Default Last modified by: Conference Room Lpt Created Date
Title: General Astrophysical Concepts: Astronomical length scales and time scales Author: Default Last modified by: Conference Room Lpt Created Date
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Introduction to Astrophysical Gas Dynamics PowerPoint PPT Presentation
Introduction to Astrophysical Gas Dynamics - Solar Oscillations. Large-Scale. Structure. Simple (linear) waves. Properties: Small perturbations of velocity, density and pressure ...
Solar Oscillations. Large-Scale. Structure. Simple (linear) waves. Properties: Small perturbations of velocity, density and pressure ...
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Introduction to Astrophysical Gas Dynamics PowerPoint PPT Presentation
Introduction to Astrophysical Gas Dynamics - The marble-tube analogy for shocks. What do we learn from this analogy? ... state (2) is uniquely determined by pre-shock (1) state! ...
The marble-tube analogy for shocks. What do we learn from this analogy? ... state (2) is uniquely determined by pre-shock (1) state! ...
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Magnetic dynamo over different astrophysical scales PowerPoint PPT Presentation
Magnetic dynamo over different astrophysical scales - 10,000 galaxies for 1 Gyr, 1044 erg/s each ... Growth rate, applied to galaxy. l=2x10-9 yr-1. urms=10 km/s. kf=2p/70 pc=0.1 pc-1. urmskf=10-6 s-1 ...
10,000 galaxies for 1 Gyr, 1044 erg/s each ... Growth rate, applied to galaxy. l=2x10-9 yr-1. urms=10 km/s. kf=2p/70 pc=0.1 pc-1. urmskf=10-6 s-1 ...
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Center for Astrophysical Sciences at Johns Hopkins University 1 PowerPoint PPT Presentation
Center for Astrophysical Sciences at Johns Hopkins University 1 - Double Imaging Spectrograph. Simultaneous red and blue spectra. 3600 to 8000 0.8 to 3 /pixel. GrIm II infrared imager and spectrograph. 1 m to 2.5 m ...
Double Imaging Spectrograph. Simultaneous red and blue spectra. 3600 to 8000 0.8 to 3 /pixel. GrIm II infrared imager and spectrograph. 1 m to 2.5 m ...
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Some Astrophysical Implications from Dark Matter Neutralino Annihilation PowerPoint PPT Presentation
Some Astrophysical Implications from Dark Matter Neutralino Annihilation - Very close to the EGRET upper limit for a cluster @ 100Mpc. Many positional coincidence between clusters and un-ID EGRET sources (e.g. Reimer et al. 2003) ...
Very close to the EGRET upper limit for a cluster @ 100Mpc. Many positional coincidence between clusters and un-ID EGRET sources (e.g. Reimer et al. 2003) ...
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An Updated Library of Reaction Rates for the Astrophysical rp- Process. The importance of Nuclear Structure Effects. PowerPoint PPT Presentation
An Updated Library of Reaction Rates for the Astrophysical rp- Process. The importance of Nuclear Structure Effects. - Title: An Updated Library of Reaction Rates for the Astrophysical rp- Process. The importance of Nuclear Structure Effects. Author: sakharuk Last modified by
Title: An Updated Library of Reaction Rates for the Astrophysical rp- Process. The importance of Nuclear Structure Effects. Author: sakharuk Last modified by
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COSMOLOGY 566 Astrophysical Constraints on Particle Physics PowerPoint PPT Presentation
COSMOLOGY 566 Astrophysical Constraints on Particle Physics - I will choose as many different scenarios as there are groups. ... X Ray, Gamma Ray and Gravitational Wave Backgrounds. Dark Matter Density and Distribution ...
I will choose as many different scenarios as there are groups. ... X Ray, Gamma Ray and Gravitational Wave Backgrounds. Dark Matter Density and Distribution ...
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Numerical simulation of astrophysical jets and accretion disks PowerPoint PPT Presentation
Numerical simulation of astrophysical jets and accretion disks - Understanding the physics of accretion-ejection flows. is central to the understanding of ... Jet acceleration and collimation. Emission from shocks in YSO jets ...
Understanding the physics of accretion-ejection flows. is central to the understanding of ... Jet acceleration and collimation. Emission from shocks in YSO jets ...
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An Astrophysical Application of Crystalline Color Superconductivity PowerPoint PPT Presentation
An Astrophysical Application of Crystalline Color Superconductivity - 6 /12. Dispersion laws for (rd gu) and (rs bu) LOFF phase is gapless ... Dispersion laws for (ru gd bs) Bari, SMFT 20.IX.06. Anglani (U Bari) 19 /12 ...
6 /12. Dispersion laws for (rd gu) and (rs bu) LOFF phase is gapless ... Dispersion laws for (ru gd bs) Bari, SMFT 20.IX.06. Anglani (U Bari) 19 /12 ...
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Helical MagnetoRotational Instability and Issues in Astrophysical Jets PowerPoint PPT Presentation
Helical MagnetoRotational Instability and Issues in Astrophysical Jets - but jets are already prone to several vigorous instabilities. pinch, kink, Kelvin-Helmholtz, ... Astrophysical jets & outflows' ...
but jets are already prone to several vigorous instabilities. pinch, kink, Kelvin-Helmholtz, ... Astrophysical jets & outflows' ...
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LIGOs Ultimate Astrophysical Reach PowerPoint PPT Presentation
LIGOs Ultimate Astrophysical Reach - Full theory, including coating anisotropy, different mechanical properties of ... Another approximation: Neglect anisotropy in coating, different parameters ...
Full theory, including coating anisotropy, different mechanical properties of ... Another approximation: Neglect anisotropy in coating, different parameters ...
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INAFCatania Astrophysical Observatory PowerPoint PPT Presentation
INAFCatania Astrophysical Observatory - INAFCatania Astrophysical Observatory
INAFCatania Astrophysical Observatory
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Acceleration of plasma outflows from compact astrophysical sources PowerPoint PPT Presentation
Acceleration of plasma outflows from compact astrophysical sources - The theory implies magnetically-dominated flow in the vicinity of pulsar, as the ... of ideal axisymmetric magneto-hydrodynamics it is possible to accelerate ...
The theory implies magnetically-dominated flow in the vicinity of pulsar, as the ... of ideal axisymmetric magneto-hydrodynamics it is possible to accelerate ...
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Precise Spectroscopy of Astrophysically Important Species PowerPoint PPT Presentation
Precise Spectroscopy of Astrophysically Important Species - Snyder, Hollis and Buhl 1977 ApJ 215, L87. Frerking, Langer and Wilson 1979 ApJ 232, L65 ... ( Snyder L.E., Hollis J.M., and Buhl D. 1977 ApJ 215, L87: eQq(HNC) ...
Snyder, Hollis and Buhl 1977 ApJ 215, L87. Frerking, Langer and Wilson 1979 ApJ 232, L65 ... ( Snyder L.E., Hollis J.M., and Buhl D. 1977 ApJ 215, L87: eQq(HNC) ...
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Production of radiatively cooled hypersonic plasma jets and links to astrophysical jets PowerPoint PPT Presentation
Production of radiatively cooled hypersonic plasma jets and links to astrophysical jets - Production of radiatively cooled hypersonic plasma jets and links to astrophysical jets
Production of radiatively cooled hypersonic plasma jets and links to astrophysical jets
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Searching for Astrophysical Neutrinos in Coincidence with Gamma Ray Bursts PowerPoint PPT Presentation
Searching for Astrophysical Neutrinos in Coincidence with Gamma Ray Bursts - Searching for Astrophysical Neutrinos in Coincidence with Gamma ... source of the highest energy CRs. Produce pions in photomeson reactions with fireball g-rays ...
Searching for Astrophysical Neutrinos in Coincidence with Gamma ... source of the highest energy CRs. Produce pions in photomeson reactions with fireball g-rays ...
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Visualization of large astrophysical simulations datasets PowerPoint PPT Presentation
Visualization of large astrophysical simulations datasets - ... the scene includes two isosurfaces, one image and one streamline objects. ... data is displayed and can be used to set interactively the desired contour value. ...
... the scene includes two isosurfaces, one image and one streamline objects. ... data is displayed and can be used to set interactively the desired contour value. ...
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Our Group Studies Fundamental Physics through Astrophysical Techniques PowerPoint PPT Presentation
Our Group Studies Fundamental Physics through Astrophysical Techniques - Our Group Studies Fundamental Physics through Astrophysical Techniques
Our Group Studies Fundamental Physics through Astrophysical Techniques
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New insights on the physics beyond the Standard Model from astrophysical observations PowerPoint PPT Presentation
New insights on the physics beyond the Standard Model from astrophysical observations - New insights on the physics beyond the Standard Model from ... http://meetings.aps.org/link/BAPS.2005.APR.T12.7; Proceedings of the2006Joint APS/JPSMeeting, ...
New insights on the physics beyond the Standard Model from ... http://meetings.aps.org/link/BAPS.2005.APR.T12.7; Proceedings of the2006Joint APS/JPSMeeting, ...
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Megaton Water Cherenkov Detectors and Astrophysical Neutrinos PowerPoint PPT Presentation
Megaton Water Cherenkov Detectors and Astrophysical Neutrinos - A taste of UNO & astrophysics. Sources. Supernova Relic n's ... Keystone Resorts & Conference Center, Keystone, Colorado Oct. 14-16, 2004 ...
A taste of UNO & astrophysics. Sources. Supernova Relic n's ... Keystone Resorts & Conference Center, Keystone, Colorado Oct. 14-16, 2004 ...
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Recent advances in Astrophysical MHD PowerPoint PPT Presentation
Recent advances in Astrophysical MHD - ... in 2D dissipation rate. after saturation is sensitive to numerical dissipation: Code Test ... Numerical dissipation is ~1.5 times smaller with. CTU & 3rd ...
... in 2D dissipation rate. after saturation is sensitive to numerical dissipation: Code Test ... Numerical dissipation is ~1.5 times smaller with. CTU & 3rd ...
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(Some of the possible) Astrophysical origins of high energy cosmic rays PowerPoint PPT Presentation
(Some of the possible) Astrophysical origins of high energy cosmic rays - To accelerate a particle efficiently it must cross the shocks ... Observational panorama: composition. Arrival directions & clustering. H.E.S.S.. 17 h data ...
To accelerate a particle efficiently it must cross the shocks ... Observational panorama: composition. Arrival directions & clustering. H.E.S.S.. 17 h data ...
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4th IMPRS Astronomy Summer School Drawing Astrophysical Inferences from Data Sets PowerPoint PPT Presentation
4th IMPRS Astronomy Summer School Drawing Astrophysical Inferences from Data Sets - Weighted Nonlinear Least Squares Fitting. a.k.a. c2 Fitting ... (Remember to take the square root of the variances to get the standard deviations! ...
Weighted Nonlinear Least Squares Fitting. a.k.a. c2 Fitting ... (Remember to take the square root of the variances to get the standard deviations! ...
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Realization of hydrogen standard by ion implantation to study nuclear reactions with astrophysical i PowerPoint PPT Presentation
Realization of hydrogen standard by ion implantation to study nuclear reactions with astrophysical i - TERWAGNE Guy (LARN FUNDP Namur) ROSS Guy (University of Quebec INRS Varennes) ... Source : V. Quillet et al., Nucl. Instr. Meth. B83 (1993) 47. 14. LARN ...
TERWAGNE Guy (LARN FUNDP Namur) ROSS Guy (University of Quebec INRS Varennes) ... Source : V. Quillet et al., Nucl. Instr. Meth. B83 (1993) 47. 14. LARN ...
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The primordial 4He abundance: the astrophysical perspective PowerPoint PPT Presentation
The primordial 4He abundance: the astrophysical perspective - The first light nuclides were synthesized in a short time interval following the ... coincide, the abundance ratio He / H is either underestimated or overestimated ...
The first light nuclides were synthesized in a short time interval following the ... coincide, the abundance ratio He / H is either underestimated or overestimated ...
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Three-Dimensional MHD Simulation of Astrophysical Jet by CIP-MOCCT Method PowerPoint PPT Presentation
Three-Dimensional MHD Simulation of Astrophysical Jet by CIP-MOCCT Method - The acceleration and collimation mechanisms of astrophysical jets are still not ... One of the most promising model for jet launching and collimation is the MHD model. ...
The acceleration and collimation mechanisms of astrophysical jets are still not ... One of the most promising model for jet launching and collimation is the MHD model. ...
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South Pole Astrophysical Observatory Research Activities PowerPoint PPT Presentation
South Pole Astrophysical Observatory Research Activities - To study CMB polarization and SZ effect in galaxy clusters ... South Pole and Concordia should become world-class, complementary facilities ...
To study CMB polarization and SZ effect in galaxy clusters ... South Pole and Concordia should become world-class, complementary facilities ...
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The Astrophysical Origins of the ShortLived Radionuclides in the Early Solar System PowerPoint PPT Presentation
The Astrophysical Origins of the ShortLived Radionuclides in the Early Solar System - Proton, alpha particle Galactic Cosmic Rays (GCRs) spall ambient nuclei, producing SLRs ... GCR protons spall local CNO nuclei, produce 10Be. 10Be GCRs trapped ...
Proton, alpha particle Galactic Cosmic Rays (GCRs) spall ambient nuclei, producing SLRs ... GCR protons spall local CNO nuclei, produce 10Be. 10Be GCRs trapped ...
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Alfvn waves propagation in homogeneous and dusty astrophysical plasmas PowerPoint PPT Presentation
Alfvn waves propagation in homogeneous and dusty astrophysical plasmas - A low temperature plasma containing disperse particles of solid material, ... If dust particles are charged, they interact with the waves, and give rise ...
A low temperature plasma containing disperse particles of solid material, ... If dust particles are charged, they interact with the waves, and give rise ...
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Calculating the infrared spectra of hot astrophysical molecules PowerPoint PPT Presentation
Calculating the infrared spectra of hot astrophysical molecules - Calculating the infrared spectra of hot astrophysical molecules
Calculating the infrared spectra of hot astrophysical molecules
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Infrared Spectroscopy of Astrophysical Gas, Grains, and Ices with Sofia PowerPoint PPT Presentation
Infrared Spectroscopy of Astrophysical Gas, Grains, and Ices with Sofia - Infrared Spectroscopy of Astrophysical Gas, Grains, and Ices with Sofia R. D. Gehrza and E. E. Becklinb aUniversity of Minnesota bUniversities Space Research Association
Infrared Spectroscopy of Astrophysical Gas, Grains, and Ices with Sofia R. D. Gehrza and E. E. Becklinb aUniversity of Minnesota bUniversities Space Research Association
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A Case Study of Verifying and Validating an Astrophysical Simulation Code PowerPoint PPT Presentation
A Case Study of Verifying and Validating an Astrophysical Simulation Code - Investigate convergence of error with resolution ... 2.5-5 % sound speed with highest magnitude near the interface. Denser fluid ...
Investigate convergence of error with resolution ... 2.5-5 % sound speed with highest magnitude near the interface. Denser fluid ...
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Astrophysical Exotica: degenerate stars with ultrahigh magnetic fields white dwarfs, neutron stars, PowerPoint PPT Presentation
Astrophysical Exotica: degenerate stars with ultrahigh magnetic fields white dwarfs, neutron stars, - Astrophysical Exotica: degenerate stars with ultrahigh magnetic fields (white ... Pmag=3x1027 dynes/cm (1022 times larger than Pgas in solar photosphere) ...
Astrophysical Exotica: degenerate stars with ultrahigh magnetic fields (white ... Pmag=3x1027 dynes/cm (1022 times larger than Pgas in solar photosphere) ...
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New States of Strongly Interacting Astrophysical Matter PowerPoint PPT Presentation
New States of Strongly Interacting Astrophysical Matter - limit (quark masses=0), the theory can arrive. at the critical point as a fixed point known ... Weakly-coupled quark-gluon plasma above Tc (CERN announcement) ...
limit (quark masses=0), the theory can arrive. at the critical point as a fixed point known ... Weakly-coupled quark-gluon plasma above Tc (CERN announcement) ...
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EVLA Correlator P' Dewdney Dominion Radio Astrophysical Observatory Herzberg Institute of Astrophysi PowerPoint PPT Presentation
EVLA Correlator P' Dewdney Dominion Radio Astrophysical Observatory Herzberg Institute of Astrophysi - Aug/03 Treasury Board approval of submitted budget ($C 20M over ... 16384 spectral channels at widest bandwidth over the 16 GHz. Targetable sub-band feature: ...
Aug/03 Treasury Board approval of submitted budget ($C 20M over ... 16384 spectral channels at widest bandwidth over the 16 GHz. Targetable sub-band feature: ...
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36th Lige International Astrophysical Colloquium: From Optical to Millimetric Interferometry Extraga PowerPoint PPT Presentation
36th Lige International Astrophysical Colloquium: From Optical to Millimetric Interferometry Extraga - 36th Lige International Astrophysical Colloquium: From Optical to Millimetric Interferometry Extraga
36th Lige International Astrophysical Colloquium: From Optical to Millimetric Interferometry Extraga
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The Transient Radio Sky Astrophysical and Artificial PowerPoint PPT Presentation
The Transient Radio Sky Astrophysical and Artificial - The Transient Radio Sky Astrophysical and Artificial
The Transient Radio Sky Astrophysical and Artificial
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Astrophysical S(E)-factor of the 15N(p,a)12C reaction at sub-Coulomb energies via the Trojan-horse method PowerPoint PPT Presentation
Astrophysical S(E)-factor of the 15N(p,a)12C reaction at sub-Coulomb energies via the Trojan-horse method - The CNO Cycle in Stellar Nucleosynthesis The final step of the CNO cycle, 15N + p 12C + (also written 15N(p, )12C) is the subject of this research.
The CNO Cycle in Stellar Nucleosynthesis The final step of the CNO cycle, 15N + p 12C + (also written 15N(p, )12C) is the subject of this research.
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Study of nuclear reactions with astrophysical interest by using a hydrogen standard PowerPoint PPT Presentation
Study of nuclear reactions with astrophysical interest by using a hydrogen standard - Necessity of reverse kinematics. Necessity of absence of deuterium. Characteristics of H standard ... Necessity of absence of deuterium. 1H target. 2D target. q ...
Necessity of reverse kinematics. Necessity of absence of deuterium. Characteristics of H standard ... Necessity of absence of deuterium. 1H target. 2D target. q ...
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The Transient Radio Sky Astrophysical and Artificial PowerPoint PPT Presentation
The Transient Radio Sky Astrophysical and Artificial - 2. Key science programs ( level 0'): defined and disseminated ... Cherenkov radiation from neutrino interactions in lunar regolith (0.2 - 1GHz) SKA ...
2. Key science programs ( level 0'): defined and disseminated ... Cherenkov radiation from neutrino interactions in lunar regolith (0.2 - 1GHz) SKA ...
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N Tropy: A Framework for Analyzing Massive Astrophysical Datasets PowerPoint PPT Presentation
N Tropy: A Framework for Analyzing Massive Astrophysical Datasets - (happy astronomer) The Era of Sky Surveys. Paradigm shift in astronomy: Sky ... With N tropy, you can develop a tree-based algorithm in less time than it would ...
(happy astronomer) The Era of Sky Surveys. Paradigm shift in astronomy: Sky ... With N tropy, you can develop a tree-based algorithm in less time than it would ...
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Ballooning Instability: Origin of CuspShaped Coronal Structures and CME 1 Crimean Astrophysical Obse PowerPoint PPT Presentation
Ballooning Instability: Origin of CuspShaped Coronal Structures and CME 1 Crimean Astrophysical Obse - Instability (formation of plasma 'tangue') arises due to drifts of charged ... Quasi-MHD (collisionless magnetized plasma): ballooning instability arises due ...
Instability (formation of plasma 'tangue') arises due to drifts of charged ... Quasi-MHD (collisionless magnetized plasma): ballooning instability arises due ...
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Halos in a warm dark matter cosmology Astrophysical Probes of the Nature of Dark Matter, Irvine, Mar PowerPoint PPT Presentation
Halos in a warm dark matter cosmology Astrophysical Probes of the Nature of Dark Matter, Irvine, Mar - Q = ?/ v2 3/2 for collisionless particles Q can not increase. ... 3 halos. X same halo. Density profiles with vth (Avila-Reese et al. 2001) ...
Q = ?/ v2 3/2 for collisionless particles Q can not increase. ... 3 halos. X same halo. Density profiles with vth (Avila-Reese et al. 2001) ...
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COSMOLOGY 566: Cosmological and Astrophysical Constraints on Fundamental Physics in 4 dimensions PowerPoint PPT Presentation
COSMOLOGY 566: Cosmological and Astrophysical Constraints on Fundamental Physics in 4 dimensions - OF STATE, MATTER DENSITY, DARK MATTER. Feb. 18 (NOTE: CLASS ... Dark Matter Density and Distribution. Dark Energy Density and Distribution. Neutrino Background ...
OF STATE, MATTER DENSITY, DARK MATTER. Feb. 18 (NOTE: CLASS ... Dark Matter Density and Distribution. Dark Energy Density and Distribution. Neutrino Background ...
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