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M. Rauch

11 papers hereh-index 6513.9k citations260 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author1
  • first author2
  • middle author3
  • last author3

Across the 9 of 11 papers where every author was matched, so the position is known.

fields
  • astro-ph7
  • hep-ph4
same name
  • M. Rauch — 1 paper, h 7

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
19952007
most citedHow cold is cold dark matter? Small scales constraints from the flux power spectrum of the high-redshift Lyman-alpha forest

207 citations · 300 across the 4 of their papers we have counts for

collaborators
Showing 2007Show all

4 papers · 1 filter

hep-ph2007★ 2 cited

Herwig++ 2.1 Release Note

M. Bahr, S. Gieseke, M. Gigg +8

A new release of the Monte Carlo program Herwig++ (version 2.1) is now available. This version includes a number of significant improvements including: an eikonal multiple parton-p…

hep-ph2007★ 8 cited

SFitter: Reconstructing the MSSM Lagrangian from LHC data

M. Rauch, R. Lafaye, T. Plehn +1

Once supersymmetry is found at the LHC, the question arises what are the fundamental parameters of the Lagrangian. The answer to this question should thereby not be biased by assum…

hep-ph2007★ 83 cited

Measuring Supersymmetry

Remi Lafaye, Tilman Plehn, Michael Rauch +1

If new physics is found at the LHC (and the ILC) the reconstruction of the underlying theory should not be biased by assumptions about high--scale models. For the mapping of many m…

astro-ph2007★ 207 cited

How cold is cold dark matter? Small scales constraints from the flux power spectrum of the high-redshift Lyman-alpha forest

M. Viel, G. D. Becker, J. S. Bolton +3

We present constraints on the mass of warm dark matter (WDM) particles derived from the Lyman-alpha flux power spectrum of 55 high- resolution HIRES spectra at 2.0 < z < 6.4. From…

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