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NSR database version of April 11, 2024.

Search: Author = S.Schramm

Found 74 matches.

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2021MO05      Nucl.Phys. A1005, 121836 (2021)

A.Motornenko, J.Steinheimer, V.Vovchenko, S.Schramm, H.Stoecker

QCD equation of state at vanishing and high baryon density: Chiral Mean Field model

doi: 10.1016/j.nuclphysa.2020.121836
Citations: PlumX Metrics


2020MO12      Phys.Rev. C 101, 034904 (2020)

A.Motornenko, J.Steinheimer, V.Vovchenko, St.Schramm, H.Stoecker

Equation of state for hot QCD and compact stars from a mean-field approach

doi: 10.1103/PhysRevC.101.034904
Citations: PlumX Metrics


2019DE09      J.Phys.(London) G46, 035102 (2019)

V.Dexheimer, R.de Oliveira Gomes, S.Schramm, H.Pais

What do we learn about vector interactions from GW170817?

doi: 10.1088/1361-6471/ab01f0
Citations: PlumX Metrics


2019MO07      Nucl.Phys. A982, 891c (2019)

A.Motornenko, V.Vovchenko, J.Steinheimer, S.Schramm, H.Stoecker

QCD at high density: Equation of state for nuclear collisions and neutron stars

doi: 10.1016/j.nuclphysa.2018.11.028
Citations: PlumX Metrics


2019SC05      Nucl.Phys. A982, 887c (2019)

S.Schramm, J.Steinheimer, V.Dexheimer, A.Mukherjee

Modeling Hybrid Stars and Hot Matter

doi: 10.1016/j.nuclphysa.2018.09.067
Citations: PlumX Metrics


2017DE28      Nucl.Phys. A967, 780 (2017)

V.Dexheimer, M.Hempel, I.Iosilevskiy, S.Schramm

Phase transitions in dense matter

doi: 10.1016/j.nuclphysa.2017.04.031
Citations: PlumX Metrics


2017MU15      Phys.Rev. C 96, 025205 (2017)

A.Mukherjee, J.Steinheimer, S.Schramm

Higher-order baryon number susceptibilities: Interplay between the chiral and the nuclear liquid-gas transitions

doi: 10.1103/PhysRevC.96.025205
Citations: PlumX Metrics


2017NA16      Phys.Rev. C 95, 065801 (2017)

R.Nandi, S.Schramm

Effect of the Coulomb interaction on the liquid-gas phase transition of nuclear matter

doi: 10.1103/PhysRevC.95.065801
Citations: PlumX Metrics


2016NA28      Phys.Rev. C 94, 025806 (2016)

R.Nandi, S.Schramm

Low-density nuclear matter with quantum molecular dynamics: The role of the symmetry energy

NUCLEAR STRUCTURE 40Ca, 62Ni, 90Zr, 152Sm, 208Pb; calculated binding energies from simulation with three different parameter sets, and compared with experimental values. Investigated effect of isospin-dependent nuclear forces on the pasta phase in the inner crust of neutron stars, within the framework of quantum molecular dynamics (QMD), and using GPU processors for computations.

doi: 10.1103/PhysRevC.94.025806
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2015DE16      Phys.Rev. C 91, 055808 (2015)

V.Dexheimer, R.Negreiros, S.Schramm

Role of strangeness in hybrid stars and possible observables

doi: 10.1103/PhysRevC.91.055808
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2015DE18      Phys.Rev. C 92, 012801 (2015)

V.Dexheimer, R.Negreiros, S.Schramm

Reconciling nuclear and astrophysical constraints

doi: 10.1103/PhysRevC.92.012801
Citations: PlumX Metrics


2015TA15      Int.J.Mod.Phys. E24, 1550057 (2015)

V.N.Tarasov, K.A.Gridnev, S.Schramm, V.I.Kuprikov, D.K.Gridnev, D.V.Tarasov, K.S.Godbey, X.Vinas, W.Greiner

Light exotic nuclei with extreme neutron excess and 2 ≤ Z ≤ 8

NUCLEAR STRUCTURE 18He, 40C; calculated neutron and proton rms radii, density distributions. HF + BCS method.

doi: 10.1142/S0218301315500573
Citations: PlumX Metrics


2014GR09      Eur.Phys.J. A 50, 118 (2014)

D.K.Gridnev, S.Schramm, K.A.Gridnev, W.Greiner

Nuclear interactions with modern three-body forces lead to the instability of neutron matter and neutron stars

doi: 10.1140/epja/i2014-14118-6
Citations: PlumX Metrics


2014MA08      Phys.Rev. C 89, 025801 (2014)

R.Mallick, S.Schramm

Oblique magnetohydrodynamic shocks: Space-like and time-like characteristics

doi: 10.1103/PhysRevC.89.025801
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2014MA24      Phys.Rev. C 89, 045805 (2014)

R.Mallick, S.Schramm

Deformation of a magnetized neutron star

doi: 10.1103/PhysRevC.89.045805
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2014TA23      Bull.Rus.Acad.Sci.Phys. 78, 569 (2014); Izv.Akad.Nauk RAS, Ser.Fiz 78, 782 (2014)

V.N.Tarasov, K.A.Gridnev, W.Greiner, S.Schramm, D.K.Gridnev, D.V.Tarasov, X.Vinas

Investigation of the properties of nuclei with extreme neutron excess in the vicinity of neutron magic numbers

NUCLEAR STRUCTURE 240Ba, 248Gd, 250Dy, 266Pb; calculated single-particle spectra, J, π. Hartree-Fock method.

doi: 10.3103/S1062873814070235
Citations: PlumX Metrics


2013DE04      Phys.Rev. C 87, 015804 (2013)

V.Dexheimer, J.Steinheimer, R.Negreiros, S.Schramm

Hybrid stars in an SU(3) parity doublet model

doi: 10.1103/PhysRevC.87.015804
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2013HE17      Phys.Rev. C 88, 014906 (2013)

M.Hempel, V.Dexheimer, S.Schramm, I.Iosilevskiy

Noncongruence of the nuclear liquid-gas and deconfinement phase transitions

doi: 10.1103/PhysRevC.88.014906
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2013TA10      Int.J.Mod.Phys. E22, 1350009 (2013)

V.N.Tarasov, K.A.Gridnev, D.K.Gridnev, D.V.Tarasov, S.Schramm, X.Vinas, W.Greiner

Stability peninsulas on the neutron drip line

NUCLEAR STRUCTURE 40O, 74S, 108Fe, 166Zr, 238Xe, 240Ba, 42Ne, 80Ti, 112Zn, 170Ru, 172Pd, 248Gd, 266Pb; calculated binding energy, quadrupole deformation parameter, neutron and proton rms radii; deduced existence of stability peninsula. HF+BCS method with Skyrme forces.

doi: 10.1142/S0218301313500092
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2013TA24      Bull.Rus.Acad.Sci.Phys. 77, 842 (2013); Izv.Akad.Nauk RAS, Ser.Fiz 77, 927 (2013)

V.N.Tarasov, K.A.Gridnev, W.Greiner, S.Schramm, D.K.Gridnev, D.V.Tarasov, X.Vinas

Peninsula of neutron stability of nuclei in the neighborhood of neutron magic number N = 126

NUCLEAR STRUCTURE 164Sr, 166Zr, 168Mo, 170Ru, 172Pd, 178Te, 180Xe, 186Nd, 190Gd; calculated neutron separation energy, quadrupole deformation parameters, neutron and proton rms radii. Hartree-Fock method with Skyrme forces.

doi: 10.3103/S1062873813070241
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2012DE27      Eur.Phys.J. A 48, 189 (2012)

V.Dexheimer, R.Negreiros, S.Schramm

Hybrid stars in a strong magnetic field

doi: 10.1140/epja/i2012-12189-y
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2012GR15      Bull.Rus.Acad.Sci.Phys. 76, 871 (2012); Izv.Akad.Nauk RAS, Ser.Fiz 76, 971 (2012)

K.A.Gridnev, W.Greiner, V.N.Tarasov, S.Schramm, D.K.Gridnev, D.V.Tarasov, X.Vinas

Investigating the neutron and proton density distributions in extremely neutron-rich nuclei

NUCLEAR STRUCTURE 16,40O, 90,166Zr, 146,248Gd, 240Ba, 266Pb, 344Rn; calculated neutron and proton density distributions, neutron and proton rms radii. Hartree-Fock method using the Skyrme forces.

doi: 10.3103/S1062873812080138
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2012NE02      Phys.Rev. C 85, 035805 (2012)

R.Negreiros, V.A.Dexheimer, S.Schramm

Quark core impact on hybrid star cooling

doi: 10.1103/PhysRevC.85.035805
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2012RA06      Phys.Rev. C 85, 025204 (2012)

P.Rau, J.Steinheimer, S.Schramm, H.Stocker

Baryon resonances in a chiral hadronic model for the QCD equation of state

doi: 10.1103/PhysRevC.85.025204
Citations: PlumX Metrics


2012SC07      Int.J.Mod.Phys. E21, 1250047 (2012)

S.Schramm, D.Gridnev, D.V.Tarasov, V.N.Tarasov, W.Greiner

The quest for the heaviest uranium isotope

NUCLEAR STRUCTURE 320,340,354Cf, 350U, 344Rn; calculated quadrupole deformation parameters, proton and neutron density distributions, one- and two-neutron separation energies. Relativistic mean field and Skyrme-type approaches.

doi: 10.1142/S0218301312500474
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2012TA14      Bull.Rus.Acad.Sci.Phys. 76, 876 (2012); Izv.Akad.Nauk RAS, Ser.Fiz 76, 976 (2012)

V.N.Tarasov, K.A.Gridnev, W.Greiner, S.Schramm, D.K.Gridnev, D.V.Tarasov, X.Vinas

The peninsula of neutron nuclear stability in the vicinity of N = 258

NUCLEAR STRUCTURE 344,346Rn, 348Th, 350U; calculated one- and two-neutron separation energies, quadrupole deformation parameters; deduced peninsula of stable nuclei.

doi: 10.3103/S1062873812080266
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2011SA33      Phys.Rev. C 84, 014901 (2011)

E.Santini, J.Steinheimer, M.Bleicher, S.Schramm

Dimuon radiation at relativistic energies available at the CERN Super Proton Synchrotron within a (3 + 1)D hydrodynamic + cascade model

doi: 10.1103/PhysRevC.84.014901
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2011ST23      Phys.Rev. C 84, 045208 (2011)

J.Steinheimer, S.Schramm, H.Stocker

Hadronic SU(3) parity doublet model for dense matter and its extension to quarks and the strange equation of state

doi: 10.1103/PhysRevC.84.045208
Citations: PlumX Metrics


2010DE15      Phys.Rev. C 81, 045201 (2010)

V.A.Dexheimer, S.Schramm

Novel approach to modeling hybrid stars

doi: 10.1103/PhysRevC.81.045201
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2010MI28      Eur.Phys.J. A 45, 169 (2010)

A.Mishra, A.Kumar, S.Sanyal, V.Dexheimer, S.Schramm

Kaon properties in (proto-)neutron star matter

doi: 10.1140/epja/i2010-10986-x
Citations: PlumX Metrics


2010NE07      Phys.Rev. C 82, 035803 (2010)

R.Negreiros, V.A.Dexheimer, S.Schramm

Modeling hybrid stars with an SU(3) nonlinear σ model

doi: 10.1103/PhysRevC.82.035803
Citations: PlumX Metrics


2010ST04      Phys.Rev. C 81, 044913 (2010)

J.Steinheimer, V.Dexheimer, M.Bleicher, H.Petersen, S.Schramm, H.Stocker

Hydrodynamics with a chiral hadronic equation of state including quark degrees of freedom

doi: 10.1103/PhysRevC.81.044913
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2009DE53      Nucl.Phys. A827, 579c (2009)

V.A.Dexheimer, S.Schramm

Neutron Stars as a Probe for Dense Matter

doi: 10.1016/j.nuclphysa.2009.05.127
Citations: PlumX Metrics


2009MI22      Eur.Phys.J. A 41, 205 (2009)

A.Mishra, A.Kumar, S.Sanyal, S.Schramm

Kaon and antikaon optical potentials in isospin asymmetric hyperonic matter

doi: 10.1140/epja/i2009-10777-6
Citations: PlumX Metrics


2008DE05      Phys.Rev. C 77, 025803 (2008)

V.Dexheimer, S.Schramm, D.Zschiesche

Nuclear matter and neutron stars in a parity doublet model

doi: 10.1103/PhysRevC.77.025803
Citations: PlumX Metrics


2008DE08      J.Phys.(London) G35, 014060 (2008)

V.Dexheimer, S.Schramm, H.Stoecker

Neutron stars in a chiral model with finite temperature

doi: 10.1088/0954-3899/35/1/014060
Citations: PlumX Metrics


2008DE32      Eur.Phys.J. A 38, 105 (2008)

V.Dexheimer, G.Pagliara, L.Tolos, J.Schaffner-Bielich, S.Schramm

Neutron stars within the SU(2) parity doublet model

doi: 10.1140/epja/i2008-10652-0
Citations: PlumX Metrics


2008MI19      Phys.Rev. C 78, 024901 (2008)

A.Mishra, S.Schramm, W.Greiner

Kaons and antikaons in asymmetric nuclear matter

doi: 10.1103/PhysRevC.78.024901
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2008ST06      Phys.Rev. C 77, 034901 (2008)

J.Steinheimer, M.Bleicher, H.Petersen, S.Schramm, H.Stocker, D.Zschiesche

(3+1)-dimensional hydrodynamic expansion with a critical point from realistic initial conditions

doi: 10.1103/PhysRevC.77.034901
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2006MA72      Phys.Rev. C 74, 044311 (2006)

J.A.Maruhn, M.Kimura, S.Schramm, P.-G.Reinhard, H.Horiuchi, A.Tohsaki

α-cluster structure and exotic states in a self-consistent model for light nuclei

NUCLEAR STRUCTURE 4He, 8Be, 12C, 16O, 20Ne, 24Mg, 28Si, 32S, 36Ar; calculated binding energies, deformation, cluster configurations. 28Si, 32S, 36Ar, 40Ca; calculated superdeformed states features.

doi: 10.1103/PhysRevC.74.044311
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2006MI34      Phys.Rev.C 74, 064904 (2006)

A.Mishra, S.Schramm

Isospin dependent kaon and antikaon optical potentials in dense hadronic matter

doi: 10.1103/PhysRevC.74.064904
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2005ZS01      J.Phys.(London) G31, 935 (2005)

D.Zschiesche, G.Zeeb, S.Schramm, H.Stocker

Impact of baryon resonances on the chiral phase transition at finite temperature and density

doi: 10.1088/0954-3899/31/8/022
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2004BU18      Acta Phys.Hung.N.S. 19, 149 (2004)

T.Burvenich, T.Cornelius, A.Sulaksono, J.A.Maruhn, W.Greiner, D.G.Madland, P.-G.Reinhard, S.Schramm

Application and Extrapolation of Mean-Field Models in the Heavy and Superheavy Regions

NUCLEAR STRUCTURE 292120; calculated neutron and proton density distributions. Relativistic point-coupling models.

doi: 10.1556/APH.19.2004.1-2.23
Citations: PlumX Metrics


2004FL05      Eur.Phys.J. A 22, 363 (2004)

P.Fleischer, P.Klupfel, T.Cornelius, T.J.Burvenich, S.Schramm, J.A.Maruhn, P.-G.Reinhard

The two-proton shell gap in Sn isotopes

NUCLEAR STRUCTURE 108,110,112,114,116,118,120,122,124,126,128,130,132Sn; calculated two-proton shell gap, deformation and correlation effects. Cd, Sn, Te; calculated deformation energies. Several models compared.

doi: 10.1140/epja/i2004-10054-4
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2004JO17      J.Phys.(London) G30, L43 (2004)

E.F.Jones, J.H.Hamilton, P.M.Gore, A.V.Ramayya, J.K.Hwang, A.P.deLima, S.J.Zhu, Y.X.Luo, C.J.Beyer, J.Kormicki, X.Q.Zhang, W.C.Ma, I.Y.Lee, J.O.Rasmussen, S.C.Wu, T.N.Ginter, P.Fallon, M.Stoyer, J.D.Cole, A.V.Daniel, G.M.Ter-Akopian, R.Donangelo, S.J.Asztalos, T.Cornelius, P.Fleischer, M.Bender, T.Burvenich, S.Schramm, J.A.Maruhn, P.-G.Reinhard

Identification of levels in 162, 164Gd and decrease in moment of inertia between N = 98-100

RADIOACTIVITY 252Cf(SF); measured Eγ, Iγ, γγ-coin. 162,164Gd deduced levels, J, π, rotational bands. Collective features in neighboring nuclides discussed.

doi: 10.1088/0954-3899/30/12/L02
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2004MI06      Phys.Rev. C 69, 015202 (2004)

A.Mishra, E.L.Bratkovskaya, J.Schaffer-Bielich, S.Schramm, H.Stocker

Mass modification of D meson in hot hadronic matter

doi: 10.1103/PhysRevC.69.015202
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2004MI11      Phys.Rev. C 69, 024903 (2004)

A.Mishra, K.Balazs, D.Zschiesche, S.Schramm, H.Stocker, W.Greiner

Effects of Dirac sea polarization on hadronic properties: A chiral SU(3) approach

doi: 10.1103/PhysRevC.69.024903
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2004MI47      Phys.Rev. C 70, 044904 (2004)

A.Mishra, E.L.Bratkovskaya, J.Schaffner-Bielich, S.Schramm, H.Stocker

Kaons and antikaons in hot and dense hadronic matter

NUCLEAR REACTIONS Ni(Ni, K+X), (Ni, K-X), E=1.93 GeV/nucleon; 197Au(197Au, K+X), (197Au, K-X), E=1.5 GeV/nucleon; calculated kaon spectra, σ(θ), directed and elliptic flow, medium modification effects. Chiral SU(3) model, comparisons with data.

doi: 10.1103/PhysRevC.70.044904
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2004ZS01      J.Phys.(London) G30, S381 (2004)

D.Zschiesche, G.Zeeb, K.Paech, S.Schramm, H.Stocker

Particle ratios from AGS to RHIC in an interacting hadronic model

NUCLEAR REACTIONS 197Au(197Au, X), E=high; calculated particle yield ratios; deduced phase transition features. Chiral SU(3) model.

doi: 10.1088/0954-3899/30/1/046
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2004ZS03      Phys.Rev. C 70, 045202 (2004)

D.Zschiesche, A.Mishra, S.Schramm, H.Stocker, and W.Greiner

In-medium vector meson masses in a chiral SU(3) model

doi: 10.1103/PhysRevC.70.045202
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2003SC03      J.Phys.(London) G29, 531 (2003)

S.Schramm, D.Zschiesche

Rotating neutron stars in a chiral SU(3) model

doi: 10.1088/0954-3899/29/3/307
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2003SC09      Phys.Lett. B 560, 164 (2003)

S.Schramm

Nuclear and neutron star radii

NUCLEAR STRUCTURE 138Ba, 208Pb; analyzed neutron and proton radii, role of nonlinear meson couplings. Implications for neutron star radii discussed.

doi: 10.1016/S0370-2693(03)00408-8
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2002BE09      Phys.Rev. C65, 024301 (2002)

Ch.Beckmann, P.Papazoglou, D.Zschiesche, S.Schramm, H.Stocker, W.Greiner

Nuclei, Superheavy Nuclei, and Hypermatter in a Chiral SU(3) Model

NUCLEAR STRUCTURE 16O, 40Ca, 208Pb; calculated charge form factors. Z=110-124; calculated binding energies, two-nucleon separation energies. 292120; calculated radial charge distribution, α-decay energies. 12,13C, 16O, 28Si, 40Ca, 51V, 89Y, 209Pb; calculated hyperon single-particle energies. 5He, 6,7,8,9Li, 7,8,9,10Be, 10,11B, 12,13C, 15N; calculated hyperon binding energies. Chiral SU(3) model.

doi: 10.1103/PhysRevC.65.024301
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2002SC48      Phys.Rev. C 66, 064310 (2002)

S.Schramm

Deformed nuclei in a chiral model

NUCLEAR STRUCTURE Z=10-126; calculated two-nucleon gaps. 20,22,24,26,28,30,32,34,36,38,40,42Mg, 68Se, 168,170,172Dy, 172,174,176Er, 192,194Hg, 252,254,256No; calculated binding energy vs quadrupole deformation. Chiral model.

doi: 10.1103/PhysRevC.66.064310
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2002ZS01      Phys.Rev. C65, 064902 (2002)

D.Zschiesche, H.Stocker, W.Greiner, S.Schramm

Space-Time Evolution and Hanbury Brown-Twiss Analysis of Relativistic Heavy Ion Collisions in a Chiral SU(3) X SU(3) Model

NUCLEAR REACTIONS 197Au(197Au, X), E=high; calculated pion source features, dependence on equation of state. Hydrodynamics simulation, chiral SU(3) model.

doi: 10.1103/PhysRevC.65.064902
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2002ZS02      Phys.Lett. 547B, 7 (2002)

D.Zschiesche, S.Schramm, J.Schaffner-Bielich, H.Stocker, W.Greiner

Particle ratios at RHIC: Effective hadron masses and chemical freeze-out

NUCLEAR REACTIONS 197Au(197Au, X), E(cm)=130 GeV/nucleon; analyzed particle yield ratios; deduced temperature and chemical potential parameters. Chiral SU(3) approach.

doi: 10.1016/S0370-2693(02)02736-3
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2001SC57      Acta Phys.Hung.N.S. 14, 341 (2001)

S.Schramm, C.Beckmann, H.Stocker, D.Zschiesche, W.Greiner

Chiral Symmetry in Nuclei and Nuclear Matter

doi: 10.1556/APH.14.2001.1-4.32
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2001ZS01      Phys.Rev. C63, 025211 (2001)

D.Zschiesche, P.Papazoglou, S.Schramm, J.Schaffner-Bielich, H.Stocker, W.Greiner

Hadrons in Dense Resonance Matter: A chiral SU(3) approach

doi: 10.1103/PhysRevC.63.025211
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2001ZS02      Nucl.Phys. A681, 34c (2001)

D.Zschiesche, L.Gerland, S.Schramm, J.Schaffner-Bielich, H.Stocker, W.Greiner

Critical Review of Quark Gluon Plasma Signals

doi: 10.1016/S0375-9474(00)00478-4
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2000ZS01      Nucl.Phys. A663-664, 737c (2000)

D.Zschiesche, P.Papazoglou, Ch.W.Beckmann, S.Schramm, J.Schaffner-Bielich, H.Stocker, W.Greiner

Chiral Model for Dense, Hot and Strange Hadronic Matter

doi: 10.1016/S0375-9474(99)00707-1
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1999AR03      Phys.Lett. 446B, 191 (1999)

D.Ardouin, S.Soff, C.Spieles, S.A.Bass, H.Stocker, D.Gourio, S.Schramm, C.Greiner, R.Lednicky, V.L.Lyuboshitz, J.P.Coffin, C.Kuhn

Unlike Particle Correlations and the Strange Quark Matter Distillation Process

doi: 10.1016/S0370-2693(98)01566-4
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1999EI01      Phys.Rev. A59, 1223 (1999)

U.Eichmann, J.Reinhardt, S.Schramm, W.Greiner

Coulomb Effects on Electromagnetic Pair Production in Ultrarelativistic Heavy-Ion Collisions

doi: 10.1103/PhysRevA.59.1223
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1999MA30      Phys.Rev. C59, 3381 (1999)

G.Mao, P.Papazoglou, S.Hofmann, S.Schramm, H.Stocker, W.Greiner

Kaon Effective Mass and Energy from a Novel Chiral SU(3)-Symmetric Lagrangian

doi: 10.1103/PhysRevC.59.3381
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1999MA43      Prog.Part.Nucl.Phys. 42, 207 (1999)

G.Mao, P.Papazoglou, S.Hofmann, S.Schramm, H.Stocker, W.Greiner

Effective Kaon Energy from a Novel Chiral SU(3) Model

doi: 10.1016/S0146-6410(99)00075-7
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1999PA02      Phys.Rev. C59, 411 (1999)

P.Papazoglou, D.Zschiesche, S.Schramm, J.Schaffner-Bielich, H.Stocker, W.Greiner

Nuclei in a Chiral SU(3) Model

NUCLEAR STRUCTURE 16O, 40Ca, 208Pb; calculated binding energy, charge radius, charge distribution, spin-orbit splitting. Chiral SU(3) model.

doi: 10.1103/PhysRevC.59.411
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1998PA11      Phys.Rev. C57, 2576 (1998)

P.Papazoglou, S.Schramm, J.Schaffner-Bielich, H.Stocker, W.Greiner

Chiral Lagrangian for Strange Hadronic Matter

doi: 10.1103/PhysRevC.57.2576
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1997KI21      Phys.Rev. C56, 1582 (1997)

H.Kim, S.Schramm, S.H.Lee

Δ Decay in the Nuclear Medium

doi: 10.1103/PhysRevC.56.1582
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1997MI16      Phys.Rev. C56, 1380 (1997)

A.Mishra, P.K.Panda, S.Schramm, J.Reinhardt, W.Greiner

Structure of the Vacuum in Nuclear Matter: A nonperturbative approach

doi: 10.1103/PhysRevC.56.1380
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1997PA06      Phys.Rev. C55, 1499 (1997)

P.Papazoglou, J.Schaffner, S.Schramm, D.Zschiesche, H.Stocker, W.Greiner

Phase Transition in the Chiral σ-ω Model with Dilatons

doi: 10.1103/PhysRevC.55.1499
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1997SO29      J.Phys.(London) G23, 2095 (1997)

S.Soff, D.Ardouin, C.Spieles, S.A.Bass, H.Stocker, D.Gourio, S.Schramm, C.Greiner, R.Lednicky, V.L.Lyuboshitz, J.-P.Coffin, C.Kuhn

Search for the Production of Strangelets in Quark Matter using Particle Correlations

NUCLEAR REACTIONS S, 197Au(197Au, X), E=high; calculated strange quark matter particle yields, correlations. Two-phase thermodynamical model.

doi: 10.1088/0954-3899/23/12/035
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1996KI05      Phys.Rev. C53, 2468 (1996)

H.Kim, S.Schramm, C.J.Horowitz

Delta Excitations in Neutrino-Nucleus Scattering

NUCLEAR REACTIONS 16O(ν, μ), E=1 GeV; calculated double differential σ. Quasielastic scattering, Δ-hole excitation.

doi: 10.1103/PhysRevC.53.2468
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1996KI06      Phys.Rev. C53, 3131 (1996)

H.Kim, S.Schramm, C.J.Horowitz

Detection of Atmospheric Neutrinos and Relativistic Nuclear Structure Effects

doi: 10.1103/PhysRevC.53.3131
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1994SC13      Phys.Rev. C49, 2777 (1994)

S.Schramm, C.J.Horowitz

Meson Exchange Effects in Parity Violating Electron-Deuteron Scattering

NUCLEAR REACTIONS 2H(e, e'X), E not given; calculated parity violating response functions ratio, asymmetry; deduced heavy meson exchange effects contribution.

doi: 10.1103/PhysRevC.49.2777
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1994SC27      Phys.Lett. 335B, 279 (1994)

S.Schramm, C.J.Horowitz

Pion-Sigma Exchange and the Proton-Proton Fusion Rate

NUCLEAR REACTIONS 1H(p, X), E not given; calculated fusion rate in solar p+p → d+e+ν reaction; deduced π-σ meson exchange correction contribution to pp S-factor.

doi: 10.1016/0370-2693(94)90350-6
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