Neutrino masses, cosmological inflation and dark matter in a variant <i>U</i>(1)<sub>B-L</sub> model with type II seesaw mechanism

[1]
C. Patrignani et al. (Particle Data Group), Chin. Phys. C 40, 100001 (2016)
[2]
P. Minkowski, Phys. Lett. B 67, 421 (1977)
[3]
T. Yanagida, Conf. Proc. C 7902131, 95 (1979)
[4]
M. Gell-Mann, P. Ramond, and R. Slansky, Conf. Proc. C 790927, 315 (1979), arXiv:1306.4669
[5]
R. N. Mohapatra and G. Senjanovic, Phys. Rev. Lett. 44, 912 (1980), [231 (1979)]
[6]
J. Schechter and J. Valle, Phys. Rev. D 22, 2227 (1980)
[7]
S. M. Faber and J. S. Gallagher, Ann. Rev. Astron. Astrophys. 17, 135 (1979)
[8]
D. Clowe, M. Bradac, A. H. Gonzalez et al., Astrophys. J. 648, L109 (2006), arXiv:astro-ph/0608407
[9]
N. Aghanim et al. (Planck) (2018), arXiv: 1807.06209
[10]
G. Jungman, M. Kamionkowski, and K. Griest, Phys. Rept. 267, 195 (1996), arXiv:hepph/9506380
[11]
G. Bertone, D. Hooper, and J. Silk, Phys. Rept. 405, 279 (2005), arXiv:hep-ph/0404175
[12]
A. H. Guth, Phys. Rev. D 23, 347 (1981)
[13]
A. D. Linde, Phys. Lett. B 108, 389 (1982)
[14]
A. Albrecht and P. J. Steinhardt, Phys. Rev. Lett. 48, 1220 (1982)
[15]
C. L. Bennett et al. (WMAP), Astrophys. J. Suppl. 208, 20 (2013), arXiv:1212.5225
[16]
N. Makino and M. Sasaki, Prog. Theor. Phys. 86, 103 (1991)
[17]
F. L. Bezrukov and M. Shaposhnikov, Phys. Lett. B 659, 703 (2008), arXiv:0710.3755
[18]
R. N. Mohapatra and R. E. Marshak, Phys. Rev. Lett. 44, 1316 (1980), [Erratum: Phys. Rev. Lett. 44, 1643 (1980)]
[19]
T. Appelquist, B. A. Dobrescu, and A. R. Hopper, Phys. Rev. D 68, 035012 (2003), arXiv:hepph/0212073
[20]
L. Basso, A. Belyaev, S. Moretti et al., Phys. Rev. D 80, 055030 (2009), arXiv:0812.4313
[21]
S. Khalil, Phys. Rev. D 82, 077702 (2010), arXiv:1004.0013
[22]
N. Okada, M. U. Rehman, and Q. Shafi, Phys. Lett. B 701, 520 (2011), arXiv:1102.4747
[23]
X. G. He, G. C. Joshi, H. Lew et al., Phys. Rev. D 43, 22 (1991)
[24]
X.-G. He, G. C. Joshi, H. Lew et al., Phys. Rev. D 44, 2118 (1991)
[25]
E. Ma, Phys. Lett. B 433, 74 (1998)
[26]
H. S. Goh, R. N. Mohapatra, and S. Nasri, Phys. Rev. D 70, 075022 (2004), arXiv:hep-ph/0408139
[27]
M. Fukugita and T. Yanagida, Phys. Lett. B 174, 45 (1986)
[28]
S. K. Majee and N. Sahu, Phys. Rev. D 82, 053007 (2010), arXiv:1004.0841
[29]
T. Nomura and H. Okada, Phys. Lett. B 774, 575 (2017), arXiv:1704.08581
[30]
R. N. Mohapatra and G. Senjanović, Phys. Rev. D 23, 165 (1981)
[31]
A. Arhrib, R. Benbrik, M. Chabab et al., Phys. Rev. D 84, 095005 (2011), arXiv:1105.1925
[32]
N. Haba, H. Ishida, N. Okada et al., Eur. Phys. J. C 76, 333 (2016), arXiv:1601.05217
[33]
C. Bonilla, R. M. Fonseca, and J. W. F. Valle, Phys. Rev. D 92, 075028 (2015), arXiv:1508.02323
[34]
J. P. Pinheiro and C. A. d. S. Pires (2020), arXiv: 2003.02350
[35]
M. Carena, A. Daleo, B. A. Dobrescu et al., Phys. Rev. D 70, 093009 (2004), arXiv:hep-ph/0408098
[36]
D. S. Salopek, J. R. Bond, and J. M. Bardeen, Phys. Rev. D 40, 1753 (1989)
[37]
R. Fakir and W. G. Unruh, Phys. Rev. D 41, 1783 (1990)
[38]
A. O. Barvinsky, A. Yu. Kamenshchik, and A. A. Starobinsky, JCAP 0811, 021 (2008), arXiv:0809.2104
[39]
J. Garcia-Bellido, D. G. Figueroa, and J. Rubio, Phys. Rev. D 79, 063531 (2009), arXiv:0812.4624
[40]
F. Bezrukov and M. Shaposhnikov, Phys. Lett. B 734, 249 (2014), arXiv:1403.6078
[41]
H. M. Lee, Phys. Rev. D 98, 015020 (2018), arXiv:1802.06174
[42]
R. N. Lerner and J. McDonald, Phys. Rev. D 80, 123507 (2009), arXiv:0909.0520
[43]
N. Okada, M. U. Rehman, and Q. Shafi, Phys. Rev. D 82, 043502 (2010), arXiv:1005.5161
[44]
M. Fairbairn, R. Hogan, and D. J. E. Marsh, Phys. Rev. D 91, 023509 (2015), arXiv:1410.1752
[45]
C. P. Burgess, H. M. Lee, and M. Trott, JHEP 09, 103 (2009), arXiv:0902.4465
[46]
J. L. F. Barbon and J. R. Espinosa, Phys. Rev. D 79, 081302 (2009), arXiv:0903.0355
[47]
C. P. Burgess, H. M. Lee, and M. Trott, JHEP 07, 007 (2010), arXiv:1002.2730
[48]
M. P. Hertzberg, JHEP 11, 023 (2010), arXiv:1002.2995
[49]
R. N. Lerner and J. McDonald, JCAP 1004, 015 (2010), arXiv:0912.5463
[50]
F. Bezrukov, Class. Quant. Grav. 30, 214001 (2013), arXiv:1307.0708
[51]
J. Rubio, Front. Astron. Space Sci. 5, 50 (2019), arXiv:1807.02376
[52]
J. G. Ferreira, C. A. de S. Pires, J. G. Rodrigues et al., Phys. Rev. D 96, 103504 (2017), arXiv:1707.01049
[53]
C.-S. Chen and C.-M. Lin, Phys. Lett. B 695, 9 (2011), arXiv:1009.5727
[54]
C. Arina, J.-O. Gong, and N. Sahu, Nucl. Phys. B 865, 430 (2012), arXiv:1206.0009
[55]
O. Lebedev and H. M. Lee, Eur. Phys. J. C 71, 1821 (2011), arXiv:1105.2284
[56]
G. Ballesteros, J. Redondo, A. Ringwald et al., Phys. Rev. Lett. 118, 071802 (2017), arXiv:1608.05414
[57]
S. R. Coleman and E. J. Weinberg, Phys. Rev. D 7, 1888 (1973)
[58]
M. Sher, Phys. Rept. 179, 273 (1989)
[59]
N. D. Birrell and P. C. W. Davies, Quantum Fields in Curved Space, Cambridge Monographs on Mathematical Physics, (Cambridge Univ. Press, Cambridge, UK, 1984), ISBN 0521278589, 9780521278584, 9780521278584
[60]
A. J. Accioly, U. F. Wichoski, S. F. Kwok et al., Class. Quant. Grav. 10, L215 (1993)
[61]
V. Faraoni, E. Gunzig, and P. Nardone, Fund. Cosmic Phys. 20, 121 (1999), arXiv:gr-qc/9811047
[62]
A. Linde, M. Noorbala, and A. Westphal, JCAP 1103, 013 (2011), arXiv:1101.2652
[63]
A. R. Liddle and D. H. Lyth, Cosmological inflation and large scale structure (2000), ISBN 0521575982, 9780521575980, 9780521828499
[64]
G. Ballesteros, J. Redondo, A. Ringwald et al., JCAP 1708, 001 (2017), arXiv:1610.01639
[65]
J. P. B. Almeida, N. Bernal, J. Rubio et al., JCAP 1903, 012 (2019), arXiv:1811.09640
[66]
A. R. Liddle and S. M. Leach, Phys. Rev. D 68, 103503 (2003), arXiv:astro-ph/0305263
[67]
J.-O. Gong, S. Pi, and G. Leung, JCAP 05, 027 (2015), arXiv:1501.03604
[68]
L. F. Abbott, E. Farhi, and M. B. Wise, Phys. Lett. B 117, 29 (1982)
[69]
A. D. Linde, Contemp. Concepts Phys. 5, 1 (1990), arXiv:hep-th/0503203
[70]
R. Allahverdi, R. Brandenberger, F.-Y. Cyr-Racine et al., Ann. Rev. Nucl. Part. Sci. 60, 27 (2010), arXiv:1001.2600
[71]
Y. Ema, R. Jinno, K. Mukaida et al., JCAP 1702, 045 (2017), arXiv:1609.05209
[72]
G. Belanger, F. Boudjema, A. Pukhov et al., Nuovo Cim. C033N2, 111 (2010), arXiv:1005.4133
[73]
F. Staub (2008), arXiv: 0806.0538
[74]
F. Staub, Comput. Phys. Commun. 182, 808 (2011), arXiv:1002.0840
[75]
F. Staub, Comput. Phys. Commun. 184, 1792 (2013), arXiv:1207.0906
[76]
F. Staub, Comput. Phys. Commun. 185, 1773 (2014), arXiv:1309.7223
[77]
W. Porod and F. Staub, Comput. Phys. Commun. 183, 2458 (2012), arXiv:1104.1573
[78]
W. Porod, Comput. Phys. Commun. 153, 275 (2003), arXiv:hep-ph/0301101
[79]
G. Aad et al. (ATLAS), Phys. Rev. D 90, 052005 (2014), arXiv:1405.4123
[80]
D. G. Cerdeno and A. M. Green, pp. 347-369 (2010), arXiv: 1002.1912
[81]
G. Arcadi, M. Dutra, P. Ghosh et al., Eur. Phys. J. C 78, 203 (2018), arXiv:1703.07364
[82]
F. S. Queiroz, PoS EPS-HEP2017, 080 (2017), arXiv:1711.02463
[83]
T. Marrodn Undagoitia and L. Rauch, J. Phys. G 43, 013001 (2016), arXiv:1509.08767
[84]
A. Berlin, D. Hooper, and S. D. McDermott, Phys. Rev. D 89, 115022 (2014), arXiv:1404.0022
[85]
M. Dutra, C. A. de S. Pires, and P. S. Rodrigues da Silva, JHEP 09, 147 (2015), arXiv:1504.07222
[86]
E. Aprile et al. (2018), arXiv: 1805.12562
[87]
D. S. Akerib et al. (LUX), Phys. Rev. Lett. 118, 021303 (2017), arXiv:1608.07648
[88]
E. Aprile et al. (XENON), JCAP 1604, 027 (2016), arXiv:1512.07501
[89]
C. E. Aalseth et al., Eur. Phys. J. Plus 133, 131 (2018), arXiv:1707.08145
[90]
D. S. Akerib et al. (LZ) (2015), arXiv: 1509.02910
[91]
J. Billard, L. Strigari, and E. Figueroa-Feliciano, Phys. Rev. D 89, 023524 (2014), arXiv:1307.5458
[92]
P. Creminelli, D. L. Lpez Nacir, M. Simonović et al., JCAP 11, 031 (2015), arXiv:1502.01983