Class information for: |
Basic class information |
| Class id | #P | Avg. number of references |
Database coverage of references |
|---|---|---|---|
| 20177 | 473 | 39.1 | 54% |
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 |
| 20177 | 1 | PRIMORDIAL BLACK HOLES//UMR 6083 CNRS//VERY HIGH ENERGY BURSTS | 473 |
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 BLACK HOLES | authKW | 1686380 | 10% | 57% | 46 |
| 2 | UMR 6083 CNRS | address | 129112 | 0% | 100% | 2 |
| 3 | VERY HIGH ENERGY BURSTS | authKW | 129112 | 0% | 100% | 2 |
| 4 | GRAV PARTICLE COSMOL GRPCHIKUSA KU | address | 86073 | 0% | 67% | 2 |
| 5 | EARLY UNIVERSE CEU | address | 72983 | 2% | 10% | 11 |
| 6 | ACCRETION OF RADIATION | authKW | 64556 | 0% | 100% | 1 |
| 7 | ANTIMONOPOLE ELECTRON TEMPERATURE | authKW | 64556 | 0% | 100% | 1 |
| 8 | CHALMERS TEKNISKA HGSK | address | 64556 | 0% | 100% | 1 |
| 9 | CMB DISTORTION | authKW | 64556 | 0% | 100% | 1 |
| 10 | CODE SN3 | address | 64556 | 0% | 100% | 1 |
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 | Physics, Particles & Fields | 14657 | 58% | 0% | 272 |
| 2 | Astronomy & Astrophysics | 14223 | 71% | 0% | 336 |
| 3 | Physics, Multidisciplinary | 663 | 18% | 0% | 87 |
| 4 | Physics, Nuclear | 593 | 11% | 0% | 53 |
| 5 | Multidisciplinary Sciences | 24 | 1% | 0% | 7 |
| 6 | COMPUTER APPLICATIONS & CYBERNETICS | 23 | 0% | 0% | 1 |
| 7 | Education, Scientific Disciplines | 14 | 1% | 0% | 5 |
| 8 | Instruments & Instrumentation | 7 | 2% | 0% | 10 |
| 9 | Physics, Mathematical | 1 | 1% | 0% | 5 |
| 10 | Automation & Control Systems | 1 | 1% | 0% | 3 |
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 | UMR 6083 CNRS | 129112 | 0% | 100% | 2 |
| 2 | GRAV PARTICLE COSMOL GRPCHIKUSA KU | 86073 | 0% | 67% | 2 |
| 3 | EARLY UNIVERSE CEU | 72983 | 2% | 10% | 11 |
| 4 | CHALMERS TEKNISKA HGSK | 64556 | 0% | 100% | 1 |
| 5 | CODE SN3 | 64556 | 0% | 100% | 1 |
| 6 | GEOPHYS PLANETARY PHYS PHYS PROGRAM | 64556 | 0% | 100% | 1 |
| 7 | HEP THEORY | 64556 | 0% | 100% | 1 |
| 8 | IAMDPTO FISDPTO ELECT CUCEIITPHD CUCE HYS MAT | 64556 | 0% | 100% | 1 |
| 9 | KASHIRSKOE SH 31 | 64556 | 0% | 100% | 1 |
| 10 | MADINGLEY 4 | 64556 | 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 | PHYSICAL REVIEW D | 17629 | 29% | 0% | 138 |
| 2 | JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 11216 | 7% | 1% | 31 |
| 3 | ASTROPARTICLE PHYSICS | 6239 | 3% | 1% | 14 |
| 4 | GRAVITATION & COSMOLOGY | 2345 | 1% | 1% | 4 |
| 5 | ASTRONOMICHESKII ZHURNAL | 1943 | 2% | 0% | 8 |
| 6 | ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS | 1785 | 2% | 0% | 8 |
| 7 | PHYSICS TEACHER | 1439 | 1% | 1% | 3 |
| 8 | CLASSICAL AND QUANTUM GRAVITY | 1325 | 3% | 0% | 15 |
| 9 | INTERNATIONAL JOURNAL OF MODERN PHYSICS D | 1265 | 2% | 0% | 8 |
| 10 | PHYSICS OF ATOMIC NUCLEI | 886 | 2% | 0% | 9 |
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 | CARR, BJ , KOHRI, K , SENDOUDA, Y , YOKOYAMA, J , (2010) NEW COSMOLOGICAL CONSTRAINTS ON PRIMORDIAL BLACK HOLES.PHYSICAL REVIEW D. VOL. 81. ISSUE 10. P. - | 123 | 53% | 181 |
| 2 | CARR, B , KUHNEL, F , SANDSTAD, M , (2016) PRIMORDIAL BLACK HOLES AS DARK MATTER.PHYSICAL REVIEW D. VOL. 94. ISSUE 8. P. - | 112 | 48% | 2 |
| 3 | KHLOPOV, MY , (2010) PRIMORDIAL BLACK HOLES.RESEARCH IN ASTRONOMY AND ASTROPHYSICS. VOL. 10. ISSUE 6. P. 495 -528 | 103 | 48% | 50 |
| 4 | KHLOPOV, M , (2013) FUNDAMENTAL PARTICLE STRUCTURE IN THE COSMOLOGICAL DARK MATTER.INTERNATIONAL JOURNAL OF MODERN PHYSICS A. VOL. 28. ISSUE 29. P. - | 98 | 38% | 17 |
| 5 | NAKAMA, T , (2014) THE DOUBLE FORMATION OF PRIMORDIAL BLACK HOLES.JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS. VOL. . ISSUE 10. P. - | 37 | 70% | 4 |
| 6 | NAKAMA, T , SILK, J , KAMIONKOWSKI, M , (2017) STOCHASTIC GRAVITATIONAL WAVES ASSOCIATED WITH THE FORMATION OF PRIMORDIAL BLACK HOLES.PHYSICAL REVIEW D. VOL. 95. ISSUE 4. P. - | 49 | 51% | 0 |
| 7 | CHISHOLM, JR , (2006) CLUSTERING OF PRIMORDIAL BLACK HOLES: BASIC RESULTS.PHYSICAL REVIEW D. VOL. 73. ISSUE 8. P. - | 44 | 69% | 20 |
| 8 | KOPP, M , HOFMANN, S , WELLER, J , (2011) SEPARATE UNIVERSES DO NOT CONSTRAIN PRIMORDIAL BLACK HOLE FORMATION.PHYSICAL REVIEW D. VOL. 83. ISSUE 12. P. - | 29 | 71% | 15 |
| 9 | NAYAK, B , MAJUMDAR, AS , SINGH, LP , (2010) ASTROPHYSICAL CONSTRAINTS ON PRIMORDIAL BLACK HOLES IN BRANS-DICKE THEORY.JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS. VOL. . ISSUE 8. P. - | 32 | 68% | 3 |
| 10 | CLESSE, S , GARCIA-BELLIDO, J , (2015) MASSIVE PRIMORDIAL BLACK HOLES FROM HYBRID INFLATION AS DARK MATTER AND THE SEEDS OF GALAXIES.PHYSICAL REVIEW D. VOL. 92. ISSUE 2. P. - | 39 | 39% | 12 |
Classes with closest relation at Level 1 |