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U. Geppert

4 papers hereh-index 5128 citations8 works total

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

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

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph2
  • astro-ph.HE2
same name
  • U. Geppert — 35 papers, h 27
  • U. Geppert — 5 papers

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
20002024
most citedCharting the temperature of the Hot Neutron Star in a Soft X-ray Transient

118 citations · 149 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.HE2024

Heating of Millisecond Pulsars by Magnetic Field Decay

U. Geppert

Millisecond pulsars (MSPs) are believed to be very old neutron stars (NSs) whose age may exceed significantly 108 yrs. Although cooling scenarios of isolated NSs predict for tha…

astro-ph.HE2021★ 31 cited

Rapid Modification of Neutron Star Surface Magnetic Field: A proposed mechanism for explaining Radio Emission State Changes in Pulsars

U. Geppert, R. Basu, D. Mitra +2

The radio emission in many pulsars show sudden changes, usually within a period, that cannot be related to the steady state processes within the inner acceleration region (IAR) abo…

astro-ph2005

Comment on ``The linear instability of magnetic Taylor-Couette flow with Hall effect''

M. Rheinhardt, U. Geppert

In the paper we comment on (Rüdiger & Shalybkov, Phys. Rev. E. 69, 016303 (2004) (RS)), the instability of the Taylor--Couette flow interacting with a homogeneous background field…

astro-ph2000★ 118 cited

Charting the temperature of the Hot Neutron Star in a Soft X-ray Transient

Monica Colpi, Ulrich Geppert, Dany Page +1

We explore the thermal evolution of a neutron star undergoing episodes of intense accretion, separated by long periods of quiescence. By using an exact cooling code we follow in de…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.