Published November 12, 2012 | Version v1
Journal article

Comparison of nuclear mass models at nuclearmasses.org

  • 1. Nuclear Engineering Division, Argonne National Laboratory, Argonne, Illinois, 60439 (United States)
  • 2. Japan Atomic Energy Agency, Tokai, Naka-gun, Ibaraki, 319-1195 (Japan)
  • 3. Computer Science and Mathematics Division, Oak Ridge National Lab, Oak Ridge, Tennessee, 37831-6354 (United States) and Physics Division, Oak Ridge National Lab, Oak Ridge, Tennessee, 37831-6354 (United States)
  • 4. Physics Division, Oak Ridge National Lab, Oak Ridge, Tennessee, 37831-6354 (United States)

Description

Nuclear masses are crucial in many astrophysics studies, as well as other areas of basic and applied nuclear science. There are now many different global theoretical models of nuclear masses – but choosing the best model for a given application can be challenging. The suite of codes online at nuclearmasses.org greatly facilitates the comparison of nuclear models with evaluated masses as well as the intercomparison of theoretical models. We demonstrate the utility of this suite by comparing the RMS deviations of 13 different theoretical mass models from the AME2003 evaluated masses over mass ranges appropriate for astrophysics.

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
1484
Journal Issue
1
Journal Page Range
p. 421-423
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
Conference on origin of matter and evolution of galaxies 2011
Dates
14-17 Nov 2011
Place
Wako (Japan)

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
44034868
Subject category
S73: NUCLEAR PHYSICS AND RADIATION PHYSICS; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
ASTRONOMY; ASTROPHYSICS; COMPARATIVE EVALUATIONS; COMPUTER CODES; MASS; NUCLEAR MODELS
Descriptors DEC
EVALUATION; MATHEMATICAL MODELS; PHYSICS

Optional Information

Notes
(c) 2012 American Institute of Physics