Cited by 109

The DOI matches its Crossref record; 3 of the 3 references it cites were found in a registry or an index.

Why should we care about the top quark Yukawa coupling?

Bezrukov, F., Shaposhnikov, M.·2015·Journal of Experimental and Theoretical Physics

Overview

The claims and statistics of this paper haven’t been checked yet.

Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.

A few free checks a day · papers already verified open instantly · results are public

Integrity signals

Registry

Crossref · 10.1134/s1063776115030152

Cites

3 of 3 references verified0 citation errors · 0 not checkable

Statistics

Verification

Claims the paper makes

The claims and statistics of this paper haven’t been checked yet.

Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.

A few free checks a day · papers already verified open instantly · results are public

Claims other papers make about this one

Each is checked against this paper’s own text: does it say what the citing paper says it does?

  • Within the standard model of particle physics, the present vacuum state of the universe may not be stable but only metastable, with another lower energy state at high expectation values of the Higgs field.

    “Nevertheless, the recent discovery of the Higgs boson [1,2] raises the possibility that, even within the standard model of particle physics, the present vacuum state of the universe may not be stable, but only metastable, with another lower energy state at high expectation values of the Higgs field [3][4][5][6][7].”

    From Vacuum metastability with black holes (2015) · cites this paper as [5]

Self-check

Percentages, sums and reported differences re-computed from the paper’s own numbers.

The self-check needs the paper’s full text.

Citations

Cites

Flagged first, then by citations

Research works printed but not linked: 60

  1. G. F. Giudice, arXiv:0801.2562 [hep-ph]. · arXiv
  2. G. F. Giudice, in Proceedings of the 2013 Europhysics Conference on High Energy Physics (EPS), Stockholm, Sweden, July 18–24, 2013 (Stockholm, 2013), p. 163. arXiv:1307.7879 [hep-ph]. · arXiv
  3. L. Maiani, G. Parisi, and R. Petronzio, Nucl. Phys. B 136, 115 (1978). · DOI
  4. N. Cabibbo, L. Maiani, G. Parisi, and R. Petronzio, Nucl. Phys. B 158, 295 (1979). · DOI
  5. M. Lindner, Z. Phys. C: Part. Fields 31, 295 (1986). · DOI
  6. N. V. Krasnikov, Yad. Fiz. 28, 549 (1978).
  7. P. Q. Hung, Phys. Rev. Lett. 42, 873 (1979). · DOI
  8. H. D. Politzer and S. Wolfram, Phys. Lett. B 82, 242 (1979). · DOI
  9. V. Branchina and E. Messina, Phys. Rev. Lett. 111, 241801 (2013). arXiv:1307.5193 [hep-ph]. · DOI · Paper page
  10. K. Olive et al. [Particle Data Group], Chin. Phys. C 38, 090001 (2014). · DOI
  11. J. Elias-Miro, J. R. Espinosa, G. F. Giudice, G. Isidori, A. Riotto, and A. Strumia, Phys. Lett. B 709, 222 (2012). arXiv:1112.3022 [hep-ph]. · DOI · Paper page
  12. A. Kobakhidze and A. Spencer-Smith, Phys. Lett. B 722, 130 (2013). arXiv:1301.2846 [hep-ph]. · DOI
  13. K. Enqvist, T. Meriniemi, and S. Nurmi, J. Cosmol. Astropart. Phys. 1407, 025 (2014). arXiv:1404.3699 [hep-ph]. · DOI
  14. M. Herranen, T. Markkanen, S. Nurmi, and A. Rajantie, Rhys. Rev. Lett. 113, 211102 (2014), arXiv: 1407.3141 [hep-ph]. · DOI
  15. K. Kamada (2014), arXiv:1409.5078 [hep-ph]. · arXiv
  16. P. Ade et al. [BICEP2 Collab.], Phys. Rev. Lett. 112, 241101 (2014). arXiv:1403.3985 [astro-ph.CO]. · DOI
  17. F. L. Bezrukov and M. Shaposhnikov, Phys. Lett. B 659, 703 (2008). arXiv:0710.3755 [hep-th]. · DOI
  18. T. Asaka and M. Shaposhnikov, Phys. Lett. B 620, 17 (2005). arXiv:hep-ph/0505013. · DOI
  19. T. Asaka, S. Blanchet, and M. Shaposhnikov, Phys. Lett. B 631, 151 (2005). arXiv:hep-ph/0503065. · DOI
  20. M. Shaposhnikov and I. Tkachev, Phys. Lett. B 639, 414 (2006). arXiv:hep-ph/0604236. · DOI
  21. F. Bezrukov and D. Gorbunov, J. High Energy Phys. 1307, 140 (2013). arXiv:1303.4395 [hep-ph]. · DOI
  22. W. Loinaz and R. Willey, Phys. Rev. D: Part., Fields 56, 7416 (1997). arXiv:hep-ph/9702321 [hep-ph]. · DOI
  23. A. Andreassen, W. Frost, and M. D. Schwartz, Phys. Rev. Lett. 113, 241801 (2014); arXiv:1408.0292 [hepph]. · DOI · Paper page
  24. N. Nielsen, Phys. Rev. D 90, 036008 (2014) arXiv:1406.0788 [hep-ph]. · DOI
  25. C.-S. Chen and Y. Tang, J. High Energy Phys. 1204, 019 (2012). arXiv:1202.5717 [hep-ph]. · DOI
  26. J. Elias-Miro, J. R. Espinosa, G. F. Giudice, H. M. Lee, and A. Strumia, J. High Energy Phys. 1206, 031 (2012). arXiv:1203.0237 [hep-ph]. · DOI
  27. S. Baek, P. Ko, W.-I. Park, and E. Senaha, J. High Energy Phys. 1211, 116 (2012). arXiv:1209.4163 [hepph]. · DOI
  28. K. Allison, J. High Energy Phys. 1305, 009 (2013). arXiv:1210.6852 [hep-ph]. · DOI
  29. S. Kanemura, T. Matsui, and T. Nabeshima, Phys. Lett. B 723, 126 (2013). arXiv:1211.4448 [hep-ph]. · DOI
  30. H. M. Lee, Phys. Lett. B 772, 198 (2013). arXiv:1301.1787 [hep-ph]. · DOI
  31. C. Coriano, L. Delle Rose, and C. Marzo, Phys. Lett. B 738, 13 (2014). arXiv:1407.8539 [hep-ph]. · DOI
  32. G. Bélanger, K. Kannike, A. Pukhov, and M. Raidal, J. Cosmol. Astropart. Phys. 1406, 021 (2014). arXiv:1403.4960 [hep-ph]. · DOI
  33. F. Bezrukov, M. Kalmykov, B. Kniehl, and M. Shaposhnikov, J. High Energy Phys. 1210, 140 (2012). arXiv:1205.2893 [hep-ph]. · DOI
  34. D. Buttazzo, G. Degrassi, P. P. Giardino, G. F. Giudice, F. Sala, A. Salvio, and A. Strumia, J. High Energy Phys. 1312, 089 (2014). arXiv:1307.3536 [hep-ph]. · arXiv
  35. A. Pikelner, A. Bednyakov, B. Kniehl, V. Velizhanin, and O. Veretin, in Proceedings of the 18th International Seminar on High Energy Physics (QUARKS’14), Suzdal, Russia, June 2–8, 2014 (Suzdal, 2014).
  36. L. N. Mihaila, J. Salomon, and M. Steinhauser, Phys. Rev. Lett. 108, 151602 (2012). arXiv:1201.5868 [hepph]. · DOI
  37. L. N. Mihaila, J. Salomon, and M. Steinhauser, Phys. Rev. D: Part., Fields, Gravitation, Cosmol. 86, 096008 (2012). arXiv:1208.3357 [hep-ph]. · DOI
  38. K. Chetyrkin and M. Zoller, J. High Energy Phys. 1206, 033 (2012). arXiv:1205.2892 [hep-ph]. · DOI
  39. K. Chetyrkin and M. Zoller, J. High Energy Phys. 1304, 091 (2013). arXiv:1303.2890 [hep-ph]. · DOI
  40. A. Bednyakov, A. Pikelner, and V. Velizhanin, Phys. Lett. B 722, 336 (2013). arXiv:1212.6829. · DOI
  41. A. Bednyakov, A. Pikelner, and V. Velizhanin, Nucl. Phys. B 875, 552 (2013). arXiv:1303.4364. · DOI
  42. A. Sirlin and R. Zucchini, Nucl. Phys. B 266, 389 (1986). · DOI
  43. M. Shaposhnikov, PoS EPS-HEP 2013, 155; arXiv:1311.4979 [hep-ph]. · arXiv
  44. C. Froggatt and H. B. Nielsen, Phys. Lett. B 368, 96 (1996). arXiv:hep-ph/9511371. · DOI · Paper page
  45. M. Shaposhnikov and C. Wetterich, Phys. Lett. B 683, 196 (2010). arXiv:0912.0208 [hep-th]. · DOI
  46. A. Gorsky, A. Mironov, A. Morozov, and T. Tomaras, J. Exp. Theor. Phys. 120 (2015) (in press). arXiv:1409.0492 [hep-ph]. · DOI · Paper page
  47. T. Sjostrand, S. Mrenna, and P. Z. Skands, Comput. Phys. Commun. 178, 852 (2008). arXiv:0710.3820 [hep-ph]. · DOI
  48. T. Sjostrand, S. Mrenna, and P. Z. Skands, J. High Energy Phys. 0605, 026 (2006). arXiv:hep-ph/0603175 [hep-ph]. · DOI
  49. M. Bahr, S. Gieseke, M. Gigg, D. Grellscheid, K. Hamilton, O. Latunde-Dada, S. Platzer, P. Richardson, M. H. Seymour, A. Sherstnev, J. Tully, and B.R. Webber, Eur. Phys. J. C 58, 639 (2008). arXiv:0803.0883 [hep-ph]. · DOI
  50. ATLAS Collaboration, CDF Collaboration, CMS Collaboration, D0 Collaboration (2014), ATLAS-CONF2014-008, CDF-NOTE-11071, CMS-PAS-TOP-13014, D0-NOTE-6416, arXiv:1403.4427 [hep-ex]. · arXiv
  51. Tevatron Electroweak Working Group (CDF Collaboration, D0 Collaboration) (2014), FERMILABCONF-14-227-E-TD, TEVEWWC-top2014-01, CDF-Note-6444, arXiv:1407.2682 [hep-ex]. · arXiv
  52. CMS Collaboration, (2014), CMS-PAS-TOP-14-015.
  53. S. Alekhin, A. Djouadi, and S. Moch, Phys. Lett. B 716, 214 (2012). arXiv:1207.0980 [hep-ph]. · DOI
  54. S. Frixione and A. Mitov, J. High Energy Phys. 1409, 012 (2014). arXiv:1407.2763 [hep-ph]. · DOI
  55. A. Buckley, J. Butterworth, S. Gieseke, D. Grellscheid, S. Hoche, H. Hoeth, F. Krauss, L. Lonnblad, E. Nurse, P. Richardson, S. Schumann, M. H. Seymour, T. Sjostrand, P. Skands, and B. Webber, Phys. Rep. 504, 145 (2011). arXiv:1101.2599 [hep-ph]. · DOI
  56. A. Juste, S. Mantry, A. Mitov, A. Penin, P. Skands, E. Varnes, M. Vos, and S. Wimpenny, Eur. Phys. J. C 74, 3119 (2014). arXiv:1310.0799 [hep-ph]. · DOI
  57. A. Kataev and V. Kim, Phys. Part. Nucl. 41, 946 (2010). arXiv:1001.4207 [hep-ph]. · DOI
  58. G. Bennett et al. [Muon G-2 Collab.], Phys. Rev. D: Part., Fields, Gravitation, Cosmol. 73, 072003 (2006). arXiv:hep-ex/0602035 [hep-ex]. · DOI
  59. A. Aguilar-Arevalo et al. [MiniBooNE Collab.], Phys. Rev. Lett. 102, 101802 (2009). arXiv:0812.2243 [hepex]. · DOI
  60. A. Aguilar-Arevalo et al., [LSND Collab.], Phys. Rev. D: Part., Fields 64, 112007 (2001). arXiv:hepex/0104049 [hep-ex]. · DOI

Cited by

Sorted by citations

Metadata

Authors
Bezrukov, F., & Shaposhnikov, M.
Venue
Journal of Experimental and Theoretical Physics
Published
2015-03
Volume
120
Issue
3
Pages
335-343
ISSN
  • 1063-7761
  • 1090-6509
Cited by
109
References
3
Language
en

About these checks

Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.

Statistics and arithmetic are recomputed, not judged.

Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.

What counts as a claim ›How we measure confidence ›How we check this ›

Are you an author, or do you see a problem with this page? Request a review