Class information for: |
Basic class information |
Class id | #P | Avg. number of references |
Database coverage of references |
---|---|---|---|
13571 | 828 | 45.1 | 69% |
Hierarchy of classes |
The table includes all classes above and classes immediately below the current class. |
Cluster id | Level | Cluster label | #P |
---|---|---|---|
10 | 4 | OPTICS//PHYSICS, PARTICLES & FIELDS//PHYSICS, MULTIDISCIPLINARY | 1131262 |
53 | 3 | PHYSICS, PARTICLES & FIELDS//PHYSICAL REVIEW D//ASTRONOMY & ASTROPHYSICS | 90803 |
264 | 2 | COSMIC MICROWAVE BACKGROUND//JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS//INFLATION | 19441 |
13571 | 1 | PRIMORDIAL MAGNETIC FIELDS//COSMIC MAGNETIC FIELDS THEORY//SECT MILAN BICOCCA | 828 |
Terms with highest relevance score |
rank | Term | termType | Chi square | Shr. of publ. in class containing term |
Class's shr. of term's tot. occurrences |
#P with term in class |
---|---|---|---|---|---|---|
1 | PRIMORDIAL MAGNETIC FIELDS | authKW | 1900820 | 8% | 82% | 63 |
2 | COSMIC MAGNETIC FIELDS THEORY | authKW | 743479 | 3% | 81% | 25 |
3 | SECT MILAN BICOCCA | address | 712466 | 4% | 60% | 32 |
4 | EXTRAGALACTIC MAGNETIC FIELDS | authKW | 112377 | 1% | 38% | 8 |
5 | GRP GRAVITAC COSMOL | address | 110631 | 0% | 100% | 3 |
6 | TECNOL FES ARAGON | address | 110631 | 0% | 100% | 3 |
7 | COSMOL PARTICLE PHYS PHENOMENOL | address | 77881 | 2% | 16% | 13 |
8 | BIERMANN BATTERY | authKW | 73754 | 0% | 100% | 2 |
9 | COSMOLOGICAL MAGNETIC FIELDS | authKW | 73754 | 0% | 100% | 2 |
10 | DIRACS AETHER | authKW | 73754 | 0% | 100% | 2 |
Web of Science journal categories |
Rank | Term | Chi square | Shr. of publ. in class containing term |
Class's shr. of term's tot. occurrences |
#P with term in class |
---|---|---|---|---|---|
1 | Astronomy & Astrophysics | 31119 | 79% | 0% | 656 |
2 | Physics, Particles & Fields | 29862 | 62% | 0% | 513 |
3 | Physics, Multidisciplinary | 826 | 16% | 0% | 131 |
4 | Physics, Nuclear | 671 | 9% | 0% | 76 |
5 | Physics, Fluids & Plasmas | 61 | 3% | 0% | 22 |
6 | Physics, Mathematical | 22 | 2% | 0% | 18 |
7 | Geochemistry & Geophysics | -3 | 0% | 0% | 2 |
8 | Mechanics | -3 | 0% | 0% | 4 |
9 | Computer Science, Interdisciplinary Applications | -4 | 0% | 0% | 1 |
10 | Physics, Atomic, Molecular & Chemical | -8 | 0% | 0% | 2 |
Address terms |
Rank | Term | Chi square | Shr. of publ. in class containing term |
Class's shr. of term's tot. occurrences |
#P with term in class |
---|---|---|---|---|---|
1 | SECT MILAN BICOCCA | 712466 | 4% | 60% | 32 |
2 | GRP GRAVITAC COSMOL | 110631 | 0% | 100% | 3 |
3 | TECNOL FES ARAGON | 110631 | 0% | 100% | 3 |
4 | COSMOL PARTICLE PHYS PHENOMENOL | 77881 | 2% | 16% | 13 |
5 | CR FRASCATI ROME | 36877 | 0% | 100% | 1 |
6 | ENEA CR FRASCATI ROME | 36877 | 0% | 100% | 1 |
7 | ICRA BRASIL | 36877 | 0% | 100% | 1 |
8 | MATEMAT MULTICISCIPLINARIA | 36877 | 0% | 100% | 1 |
9 | OPERAT STRATEGY CHANGE | 36877 | 0% | 100% | 1 |
10 | PHYS LYMAN | 36877 | 0% | 100% | 1 |
Journals |
Rank | Term | Chi square | Shr. of publ. in class containing term |
Class's shr. of term's tot. occurrences |
#P with term in class |
---|---|---|---|---|---|
1 | JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 49411 | 10% | 2% | 86 |
2 | PHYSICAL REVIEW D | 46465 | 36% | 0% | 296 |
3 | ASTRONOMISCHE NACHRICHTEN | 3513 | 2% | 1% | 18 |
4 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2110 | 6% | 0% | 51 |
5 | CLASSICAL AND QUANTUM GRAVITY | 1933 | 3% | 0% | 24 |
6 | PHYSICS LETTERS B | 1510 | 5% | 0% | 45 |
7 | ASTROPHYSICAL JOURNAL | 724 | 5% | 0% | 41 |
8 | INTERNATIONAL JOURNAL OF MODERN PHYSICS D | 716 | 1% | 0% | 8 |
9 | ASTROPARTICLE PHYSICS | 646 | 1% | 0% | 6 |
10 | PHYSICAL REVIEW LETTERS | 626 | 5% | 0% | 42 |
Author Key Words |
Core articles |
The table includes core articles in the class. The following variables is taken into account for the relevance score of an article in a cluster c: (1) Number of references referring to publications in the class. (2) Share of total number of active references referring to publications in the class. (3) Age of the article. New articles get higher score than old articles. (4) Citation rate, normalized to year. |
Rank | Reference | # ref. in cl. |
Shr. of ref. in cl. |
Citations |
---|---|---|---|---|
1 | KAHNIASHVILI, T , BRANDENBURG, A , TEVZADZE, AG , (2016) THE EVOLUTION OF PRIMORDIAL MAGNETIC FIELDS SINCE THEIR GENERATION.PHYSICA SCRIPTA. VOL. 91. ISSUE 10. P. - | 151 | 75% | 0 |
2 | SUBRAMANIAN, K , (2016) THE ORIGIN, EVOLUTION AND SIGNATURES OF PRIMORDIAL MAGNETIC FIELDS.REPORTS ON PROGRESS IN PHYSICS. VOL. 79. ISSUE 7. P. - | 130 | 60% | 5 |
3 | CAMPANELLI, L , (2014) EVOLUTION OF PRIMORDIAL MAGNETIC FIELDS IN MEAN-FIELD APPROXIMATION.EUROPEAN PHYSICAL JOURNAL C. VOL. 74. ISSUE 1. P. - | 113 | 88% | 6 |
4 | BAMBA, K , (2015) GENERATION OF LARGE-SCALE MAGNETIC FIELDS, NON-GAUSSIANITY, AND PRIMORDIAL GRAVITATIONAL WAVES IN INFLATIONARY COSMOLOGY.PHYSICAL REVIEW D. VOL. 91. ISSUE 4. P. - | 120 | 60% | 7 |
5 | CAMPANELLI, L , (2016) SUPERHORIZON MAGNETIC FIELDS.PHYSICAL REVIEW D. VOL. 93. ISSUE 6. P. - | 71 | 87% | 3 |
6 | CAMPANELLI, L , (2015) LORENTZ-VIOLATING INFLATIONARY MAGNETOGENESIS.EUROPEAN PHYSICAL JOURNAL C. VOL. 75. ISSUE 6. P. - | 82 | 81% | 6 |
7 | YAMAZAKI, DG , (2016) EVOLUTION OF THE COSMIC MATTER DENSITY FIELD WITH A PRIMORDIAL MAGNETIC FIELD.PHYSICAL REVIEW D. VOL. 93. ISSUE 4. P. - | 79 | 87% | 0 |
8 | TOMASI, M , TRISTRAM, M , TUCCI, M , TUOVINEN, J , UMANA, G , VALENZIANO, L , VALIVIITA, J , VAN TENT, B , VIELVA, P , VILLA, F , ET AL (2016) PLANCK 2015 RESULTS XIX. CONSTRAINTS ON PRIMORDIAL MAGNETIC FIELDS.ASTRONOMY & ASTROPHYSICS. VOL. 594. ISSUE . P. - | 87 | 72% | 1 |
9 | KANDUS, A , KUNZE, KE , TSAGAS, CG , (2011) PRIMORDIAL MAGNETOGENESIS.PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS. VOL. 505. ISSUE 1. P. 1 -58 | 118 | 46% | 118 |
10 | BAMBA, K , GENG, CQ , HO, SH , KAO, WF , (2012) LARGE-SCALE MAGNETIC FIELDS FROM INFLATION DUE TO A CPT-EVEN CHERN-SIMONS-LIKE TERM WITH KALB-RAMOND AND SCALAR FIELDS.EUROPEAN PHYSICAL JOURNAL C. VOL. 72. ISSUE 4. P. - | 89 | 78% | 2 |
Classes with closest relation at Level 1 |