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- Nora Brambilla, Simon Eidelman, +47 authors Viktor Zakharov
- The European physical journal. C, Particles andâ€¦
- 2014

We highlight the progress, current status, and open challenges of QCD-driven physics, in theory and in experiment. We discuss how the strong interaction is intimately connected to a broad sweep ofâ€¦ (More)

- Thomas Schaefer, K. Schwenzer
- Physical review letters
- 2006

We study the low-energy behavior of QCD Green functions in the limit that the baryon chemical potential is much larger than the QCD scale parameter LambdaQCD. We show that there is a systematicâ€¦ (More)

- Jens Braun, K. Schwenzer, Hans â€“ JÃ¼rgen Pirner
- 2003

We model the transition of a system of quarks and gluons at high energies to a system of quarks and mesons at low energies in a consistent renormalization group approach. Flow equations interpolateâ€¦ (More)

- Thomas Spitzenberg, K. Schwenzer
- 2009

We derive the spectrum of the Dirac operator for the linear Ïƒâ€“ model with quarks in the large Nc approximation using renormalization group flow equations. For small eigenvalues, the Banksâ€“Casherâ€¦ (More)

- Mark G. Alford, Sanjay Reddy, K. Schwenzer
- Physical review letters
- 2012

Cooper pairing between fermions in dense matter leads to the formation of a gap in the fermionic excitation spectrum and typically exponentially suppresses transport properties. However, we show hereâ€¦ (More)

- Mark G. Alford, Luke Bovard, Matthias Hanauske, Luciano Rezzolla, K. Schwenzer
- Physical review letters
- 2018

Inferring the properties of dense matter is one of the most exciting prospects from the measurement of gravitational waves from neutron star mergers. However, it requires reliable numericalâ€¦ (More)

We summarize recent results on the nonperturbative quark-gluon interaction in Landau gauge QCD. Our analytical analysis of the infrared behaviour of the quark-gluon vertex reveals infraredâ€¦ (More)

- Mark G. Alford, K. Schwenzer
- Physical review letters
- 2014

The cores of compact stars reach the highest densities in nature and therefore could consist of novel phases of matter. We demonstrate via a detailed analysis of pulsar evolution that precise pulsarâ€¦ (More)

- Jochen Meyer, K. Schwenzer, JÃ¼rgen Pirner
- 2008

We calculate renormalization group flow equations for the linear Ïƒmodel in large Nc approximation. The flow equations decouple and can be solved analytically. The solution is equal to a selfâ€¦ (More)