◍wovepaper
SearchResearchersInstitutions
Sign in
researcher

S. Schramm

47 papers hereh-index 354.1k citations281 works total

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

author position
  • sole author1
  • first author3
  • middle author25
  • last author15

Across the 44 of 47 papers where every author was matched, so the position is known.

fields
  • nucl-th27
  • hep-ph8
  • astro-ph.HE6
  • astro-ph3
  • astro-ph.SR1
  • cond-mat.mes-hall1
same name
  • S. Schramm — 273 papers
  • S. Schramm — 9 papers, h 54
  • S. Schramm — 3 papers, h 8
  • S. Schramm — 1 paper
  • S. Schramm — 1 paper, h 28
  • S. Schramm — 1 paper, h 8

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
19932020
most citedProto-Neutron and Neutron Stars in a Chiral SU(3) Model

231 citations · 908 across the 28 of their papers we have counts for

collaborators
Showing 2008Show all

4 papers · 1 filter

nucl-th2008★ 55 cited

Kaon and antikaon optical potentials in isospin asymmetric hyperonic matter

Amruta Mishra, Arvind Kumar, Sambuddha Sanyal +1

The medium modifications of the energies of kaons and antikaons in isospin asymmetric hyperonic matter are investigated using a chiral SU(3) model. The isospin dependent medium eff…

nucl-th2008★ 38 cited

Neutron stars within the SU(2) parity doublet model

V. Dexheimer, G. Pagliara, L. Tolos +2

The equation of state of beta-stable and charge neutral nucleonic matter is computed within the SU(2) parity doublet model in mean field and in the relativistic Hartree approximati…

nucl-th2008★ 49 cited

Kaons and antikaons in asymmetric nuclear matter

A. Mishra, S. Schramm, W. Greiner

The properties of kaons and antikaons and their modification in isospin asymmetric nuclear matter are investigated using a chiral SU(3) model. These isospin dependent medium effect…

astro-ph2008★ 231 cited

Proto-Neutron and Neutron Stars in a Chiral SU(3) Model

V. Dexheimer, S. Schramm

A hadronic chiral SU(3) model is applied to neutron and proto-neutron stars, taking into account trapped neutrinos, finite temperature and entropy. The transition to the chirally r…

◍wovepaper

Papers, researchers and institutions, woven together.

Explore
  • Search
  • Researchers
  • Institutions
Account
  • Library
  • Chat
Data
  • arXiv.org
  • Semantic Scholar
  • OpenAlex
  • Latest RSS
AboutContactPrivacyDevelopersllms.txtopenapi.json
Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.