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Cold Warm and Hot dark matter simulations ITP University of

Cold Warm and Hot dark matter simulations ITP University of

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Cold, Warm, and Hot dark matter simulations, ITP, University of Zurich | illustrations, measurements, instructions | Pinterest

Image credit: Liang Gao and Tom Theuns. Warm dark matter ...

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Image credit: John Peacock, via Ned Wright's cosmology tutorial.

Image credit: Adam Block / Mount Lemmon SkyCenter / University of Arizona.

Logran ver por primera vez un 'puente' de materia ...

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Cold, Warm, and Hot dark matter simulations, ITP, University of Zurich | illustrations, measurements, instructions | Pinterest | Dark matter

Image credit: NASA, ESA, and the Hubble SM4 ERO Team.

Cold, Warm, and Hot dark matter simulations, ITP, University of Zurich | illustrations, measurements, instructions | Pinterest | Dark matter

Image credit: NASA, N. Benitez (JHU), T. Broadhurst (Racah Institute of Physics/The Hebrew University), H. Ford (JHU), M. Clampin (STScI),G. Hartig (STScI), ...

Patricia Burchat: Shedding light on dark matter | Video on TED.com | My favorite TED Talks | Pinterest | Dark matter, Dark energy and Physicist

Credits: The Virgo Consortium/Alexandre Amblard/ESA | better look | Pinterest | Dark matter

Image credit: Planck Collaboration: P. A. R. Ade et al., 2013, A&A Preprint.

Image credit: Carsten A. Arnholm, of NGC 206, via http://arnholm.org/.

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Image credit: A. Sanchez / Sparke / Gallagher, 2007.

Cold, Warm, and Hot dark matter simulations, ITP, University of Zurich | illustrations, measurements, instructions | Pinterest | Dark matter

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The (dimensionless) matter power spectrum for a thermal 3.3 keV WDM (red,

Image credit: W. Percival et al. / Sloan Digital Sky Survey.

The mass fraction in substructures as a function of dimensionless radial distance from the halo centre

Images credit: ESA / Planck collaboration; P. A. R. Ade et al., 2013, A&A Preprint; annotations by me. So what is that dark matter?

Cold, Warm, and Hot dark matter simulations, ITP, University of Zurich. See more. New Measurements Suggest There May Be Half As Much Dark Matter In The ...

The z = 0 bJ- (upper panel) and K-band (lower

Cold, Warm, and Hot dark matter simulations, ITP, University of Zurich | illustrations, measurements, instructions | Pinterest | Dark matter

Cold, Warm, and Hot dark matter simulations, ITP, University of Zurich | illustrations, measurements, instructions | Pinterest | Dark matter

Image credit: NASA / COBE science team (L); unknown public domain image (R).

Cold, Warm, and Hot dark matter simulations, ITP, University of Zurich | illustrations, measurements, instructions | Pinterest | Dark matter

Cold, Warm, and Hot dark matter simulations, ITP, University of Zurich | illustrations, measurements, instructions | Pinterest | Dark matter

Cold, Warm, and Hot dark matter simulations, ITP, University of Zurich | illustrations, measurements, instructions | Pinterest | Dark matter

Cold, Warm, and Hot dark matter simulations, ITP, University of Zurich | illustrations, measurements, instructions | Pinterest | Dark matter

Cold, Warm, and Hot dark matter simulations, ITP, University of Zurich | illustrations, measurements, instructions | Pinterest | Dark matter

The subhalo rmax–Vmax relation in bins of parent halo mass (different panels)

The evolution of the UV luminosity function of all galaxies (centrals and satellites) for

Image credit: me, created at http://nces.ed.gov

Image credit: Hitoshi Murayama of http://hitoshi.berkeley.edu/.

Image credit: ESA and the Planck Collaboration.

Cold, Warm, and Hot dark matter simulations, ITP, University of Zurich | illustrations, measurements, instructions | Pinterest | Dark matter

Left-hand panel: The average stellar mass growth of all galaxies with mass 1

Cold, Warm, and Hot dark matter simulations, ITP, University of Zurich | illustrations, measurements, instructions | Pinterest | Dark matter

Sky Sighting: Is That A Thread Of Dark Matter I Spy? | Dark matter and Dark

Cold, Warm, and Hot dark matter simulations, ITP, University of Zurich | illustrations, measurements, instructions | Pinterest

Cold, Warm, and Hot dark matter simulations, ITP, University of Zurich | illustrations, measurements, instructions | Pinterest | Dark matter

The cumulative V-band luminosity function of satellites within 280 kpc of the centre of

1: Snapshots of the growth of the dark-matter halo in our

Gravitational lensing in WDM cosmologies: The cross section for giant arcs

The allowed region of parameters of sterile neutrino dark matter in the νMSM (white unshaded

Image credit: Fermi National Accelerator Laboratory (Fermi Lab), modified by me.

Stacked radial number density profiles of subhaloes, n(r), in different mass

The correlation between subhalo central mass at infall and the redshift of formation, zform,

Clusters of Galaxies

Projected density map in a slice of dimensions (70.4 × 70.4 × 1.5) h

The solid lines show the linear power spectra (from cmbfast; Seljak & Zaldarriaga 1996

Physicist Patricia Burchat sheds light on two basic ingredients of our universe: dark matter and dark energy. Comprising of the universe between them, ...

Patricia Burchat: Shedding light on dark matter | Video on TED.com | My favorite TED Talks | Pinterest | Dark matter, Dark energy and Physicist

Parameter space of sterile neutrinos responsible for neutrino oscillations (region above dotted line “neutrino

Cosmology - Dark Matter

Images of the CDM (left) and WDM (right) level 2 haloes at

The correlation between subhalo maximum circular velocity and the radius at which this maximum occurs.

Pairing of Supermassive Black Holes in galaxy mergers

Circular velocity curves for the 12 CDM (left) and WDM (right) subhaloes

via IBM STM Gallery

Properties of the Ms = 7 keV matter power spectrum as a function of L6.

Cold phase metallicity as a function of the stellar mass for model galaxies

motivation: ν s in astroparticle physics cosmic architects: role

dark matter. Top right: wa.

The free-streaming comoving distance travelled per log interval of 1 +z, where

Image credit: Andrew J. Bernstein of http://blue-mondays.blogspot.com/2010/07/vaca-pics-to-make-you-jealous.html.

Worlds Smallest Star Trek Enterprise

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Chandra Press Room :: Hot .

Example of interactions of sterile neutrino: decay N→νeναν¯α (panel (

Comparison of sensitivities of existing and proposed/planned X-ray missions for the detection

L6 as a function of the mixing angle, sin 2(2θ), for

The variation with subhalo mass at infall of the ratio of the present-day mass

The Milky Way halo mass required to account for the observed number of Milky Way satellites

Waves do not spread in a disordered medium if there is less than one wavelength between two defects. Physicists from the universities of Zurich and ...

crystal diffraction

Selected regions in the central part of M31 (shown in linear scale). Small

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Sterile neutrino momentum distributions for different values of L6 = [0, 700] as

Matter power spectra generated from the Ms = 7 keV distribution functions shown in Fig.

Anderson Localization of Light - Waves do not spread in a disordered medium if there is less than one wavelength between two defects. Physicists fr…

Of course, in a synthetic universe, we control everything, such as the laws of physics and the nature of dark matter.

nanorope: Helix formation from J., 132 pp Courtesy ACS

Standard image ...

Euclid Definition Study Report

Composite image of a galaxy cluster Canvas Art - Stocktrek Images (28 x 28)

Excluded region in the Ms–L6 plane. For sterile neutrino parameters in the cyan

Music | The Fermi Sea

What Difference Does Hot o.

is in the range 100–500 keV cm2. For the present purposes, we shall assume that the added energy increases the thermal energy of the gas (as opposed to ...

Caffeine under electron microscope

Components of the galaxy cluster Abell 2744, also known as the Pandora Cluster: galaxies (white), hot gas (red) and dark matter (blue).

Universe Dark Matter Simul.

Top panel: σ(M), the rms density fluctuation smoothed over mass scale

Cold, Warm, and Hot dark matter simulations, ITP, University of Zurich. See more. APACHE TEAR E137 Purification and Healing As the tears of the Apaches fell ...

electrostatic potential for benzene

A three colour composite Herschel Space Observatory image of the iconic Eagle Nebula, combining PACS 70 micron (blue), PACS 160 micron (green) and SPIRE 250 ...