CP³-Origins

A billowing tower of gas and dust rises from the stellar nursery known as the Eagle Nebula. This small piece of the Eagle Nebula is 57 trillion miles long (91.7 trillion km). Credit: NASA, ESA, and The Hubble Heritage Team (STScI/AURA)

A typical candidate event including two high-energy photons whose energy (depicted by red towers) is measured in the CMS electromagnetic calorimeter. The yellow lines are the measured tracks of other particles produced in the collision. The pale blue volume shows the CMS crystal calorimeter barrel. (c) CERN, CMS 2011

CERN

A view inside the liquid-argon calorimeter endcap. The circular inner bore of the EMEC, front and rear HEC wheels. (c) ATLAS

A Black Hole concept drawing (C) NASA

Radiation from hot stars off the top of the picture illuminates and erodes this giant, gaseous pillar. Additional ultraviolet radiation causes the gas to glow, giving the pillar its red halo of light. Credit: NASA, H. Ford (JHU), G. Illingworth (UCSC/LO), M.Clampin (STScI), G. Hartig (STScI), the ACS Science Team, and ESA

CP³ Black Report on the cover of EPJ Plus

M81, a spiral galaxy similar to our own Milky Way, is one of the brightest galaxies that can be seen from Earth. The spiral arms wind all the way down into the nucleus and are made up of young, bluish, hot stars formed in the past few million years, while the central bulge contains older, redder stars. Credit: NASA, ESA, and The Hubble Heritage Team (STScI/AURA)

Lowering an endcap magnet into place. (c) ATLAS

LHC Magnet Waiting for test (C) CERN

Thousands of stars are forming in the cloud of gas and dust known as the Orion nebula. More than 3,000 stars of various sizes appear in this image. Some of them have never been seen in visible light. Credit: NASA,ESA, M. Robberto (Space Telescope Science Institute/ESA) and the Hubble Space Telescope Orion Treasury Project Team

Join the CP3 World Program

Three CP³-Ph.D. students: Jakob Jark Jørgensen, Ulrik Ishøj Søndergaard, and Matin Mojaza

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News

CP3-Origins granted 22 million computing hours

Events

May 18 at 12:00: Liquid Helium and QCD: Feynman’s Last Problem

May 21 at 14:15: Effective Field Theory in Inflation