Cosmic superstrings, metastable strings and ultralight primordial black holes: from NANOGrav to LIGO and beyond

A bstract While topologically stable cosmic strings are disfavoured by the recent observation of nHz stochastic gravitational waves (GW) by Pulsar Timing Arrays (PTA), e.g., NANOGrav, cosmic metastable strings and superstrings are not. However, because the gravitational waves from all classes of str...

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Published in:The journal of high energy physics Vol. 2025; no. 2; pp. 95 - 35
Main Authors: Datta, Satyabrata, Samanta, Rome
Format: Journal Article
Language:English
Published: Berlin/Heidelberg Springer Berlin Heidelberg 14.02.2025
Springer Nature B.V
SpringerOpen
Subjects:
Baryo-and Leptogenesis
Black Holes
Classical and Quantum Gravitation
Cosmology of Theories BSM
Early Universe Particle Physics
Elementary Particles
Gravitational waves
Hawking radiation
High energy physics
LIGO (observatory)
Physics
Physics and Astronomy
Pulsars
Quantum Field Theories
Quantum Field Theory
Quantum Physics
Regular Article - Theoretical Physics
Relativity Theory
String Theory
Universe
Cosmology of Theories BSM
Black Holes
Baryo-and Leptogenesis
Early Universe Particle Physics
ISSN:1029-8479, 1029-8479
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Abstract A bstract While topologically stable cosmic strings are disfavoured by the recent observation of nHz stochastic gravitational waves (GW) by Pulsar Timing Arrays (PTA), e.g., NANOGrav, cosmic metastable strings and superstrings are not. However, because the gravitational waves from all classes of strings generally span a wide range of frequencies, they contradict LIGO’s non-observation of stochastic gravitational waves at the f ~ 25 Hz band for a substantial string-parameter space favoured by the PTA data. Suppose ultralight primordial black holes ( M BH < 10 9 g) existed in the early universe. In this case, they reduce the amplitude of the GWs at higher frequencies by providing an early matter-dominated phase, alleviating the tension between LIGO observation and PTA data. We show that the recent PTA data complemented by future LIGO-Virgo-KAGRA (LVK) runs plus detectors such as LISA and ET would be able to dapple the properties and further search strategies of such ultralight primordial black holes which are otherwise fairly elusive as they evaporate in the early universe by Hawking radiation.
AbstractList Abstract While topologically stable cosmic strings are disfavoured by the recent observation of nHz stochastic gravitational waves (GW) by Pulsar Timing Arrays (PTA), e.g., NANOGrav, cosmic metastable strings and superstrings are not. However, because the gravitational waves from all classes of strings generally span a wide range of frequencies, they contradict LIGO’s non-observation of stochastic gravitational waves at the f ~ 25 Hz band for a substantial string-parameter space favoured by the PTA data. Suppose ultralight primordial black holes (M BH < 109 g) existed in the early universe. In this case, they reduce the amplitude of the GWs at higher frequencies by providing an early matter-dominated phase, alleviating the tension between LIGO observation and PTA data. We show that the recent PTA data complemented by future LIGO-Virgo-KAGRA (LVK) runs plus detectors such as LISA and ET would be able to dapple the properties and further search strategies of such ultralight primordial black holes which are otherwise fairly elusive as they evaporate in the early universe by Hawking radiation.
While topologically stable cosmic strings are disfavoured by the recent observation of nHz stochastic gravitational waves (GW) by Pulsar Timing Arrays (PTA), e.g., NANOGrav, cosmic metastable strings and superstrings are not. However, because the gravitational waves from all classes of strings generally span a wide range of frequencies, they contradict LIGO’s non-observation of stochastic gravitational waves at the f ~ 25 Hz band for a substantial string-parameter space favoured by the PTA data. Suppose ultralight primordial black holes ( M BH < 10 9 g) existed in the early universe. In this case, they reduce the amplitude of the GWs at higher frequencies by providing an early matter-dominated phase, alleviating the tension between LIGO observation and PTA data. We show that the recent PTA data complemented by future LIGO-Virgo-KAGRA (LVK) runs plus detectors such as LISA and ET would be able to dapple the properties and further search strategies of such ultralight primordial black holes which are otherwise fairly elusive as they evaporate in the early universe by Hawking radiation.
While topologically stable cosmic strings are disfavoured by the recent observation of nHz stochastic gravitational waves (GW) by Pulsar Timing Arrays (PTA), e.g., NANOGrav, cosmic metastable strings and superstrings are not. However, because the gravitational waves from all classes of strings generally span a wide range of frequencies, they contradict LIGO’s non-observation of stochastic gravitational waves at the f ~ 25 Hz band for a substantial string-parameter space favoured by the PTA data. Suppose ultralight primordial black holes (MBH < 109 g) existed in the early universe. In this case, they reduce the amplitude of the GWs at higher frequencies by providing an early matter-dominated phase, alleviating the tension between LIGO observation and PTA data. We show that the recent PTA data complemented by future LIGO-Virgo-KAGRA (LVK) runs plus detectors such as LISA and ET would be able to dapple the properties and further search strategies of such ultralight primordial black holes which are otherwise fairly elusive as they evaporate in the early universe by Hawking radiation.
A bstract While topologically stable cosmic strings are disfavoured by the recent observation of nHz stochastic gravitational waves (GW) by Pulsar Timing Arrays (PTA), e.g., NANOGrav, cosmic metastable strings and superstrings are not. However, because the gravitational waves from all classes of strings generally span a wide range of frequencies, they contradict LIGO’s non-observation of stochastic gravitational waves at the f ~ 25 Hz band for a substantial string-parameter space favoured by the PTA data. Suppose ultralight primordial black holes ( M BH < 10 9 g) existed in the early universe. In this case, they reduce the amplitude of the GWs at higher frequencies by providing an early matter-dominated phase, alleviating the tension between LIGO observation and PTA data. We show that the recent PTA data complemented by future LIGO-Virgo-KAGRA (LVK) runs plus detectors such as LISA and ET would be able to dapple the properties and further search strategies of such ultralight primordial black holes which are otherwise fairly elusive as they evaporate in the early universe by Hawking radiation.
ArticleNumber 95
Author Datta, Satyabrata
Samanta, Rome
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Cites_doi 10.1088/1475-7516/2005/04/003
10.1103/PhysRevD.104.123536
10.1140/epjc/s10052-019-7542-5
10.1088/1475-7516/2019/11/017
10.1103/PhysRevD.106.123515
10.1103/PhysRevD.108.083527
10.1103/PhysRevLett.87.221103
10.3847/2041-8213/acdd02
10.1016/S0370-1573(99)00102-7
10.1103/PhysRevD.107.095002
10.1088/1475-7516/2021/03/053
10.1016/j.physletb.2024.138473
10.1103/PhysRevLett.101.101101
10.1007/JHEP01(2021)097
10.1103/PhysRevD.85.083525
10.1103/PhysRevLett.132.171002
10.1103/PhysRevD.95.063002
10.1093/mnras/152.1.75
10.1007/JHEP07(2022)130
10.1103/PhysRevD.109.023522
10.1007/s41114-021-00032-5
10.1088/1475-7516/2019/12/012
10.1088/1126-6708/2005/10/013
10.1103/PhysRevD.31.3052
10.1103/PhysRevD.64.064008
10.1140/epjc/s10052-020-7735-y
10.1007/JHEP05(2021)211
10.1103/PhysRevD.47.2324
10.1103/PhysRevLett.122.201301
10.3390/universe10050211
10.1007/JHEP09(2020)178
10.1103/PhysRevLett.127.231801
10.1088/1475-7516/2019/05/005
10.1103/PhysRevD.107.104021
10.1088/0264-9381/32/7/074001
10.1088/1475-7516/2021/04/062
10.1016/j.physletb.2020.135914
10.1016/j.physletb.2024.138924
10.1007/JHEP03(2023)127
10.1007/JHEP08(2019)001
10.1016/j.physletb.2023.137724
10.1088/1475-7516/2022/08/068
10.1103/PhysRevD.101.123533
10.1103/PhysRevD.73.064006
10.1007/s41114-017-0004-1
10.1103/PhysRevD.110.043528
10.1088/1475-7516/2022/10/089
10.1088/1126-6708/2004/06/013
10.1140/epjc/s10052-020-8092-6
10.1088/1475-7516/2021/08/021
10.1103/PhysRevD.104.083523
10.1017/pasa.2019.42
10.1103/PhysRevLett.126.021104
10.1088/1475-7516/2024/10/007
10.1103/PhysRevD.108.103019
10.1103/PhysRevResearch.2.043321
10.1088/1475-7516/2018/05/035
10.1088/1475-7516/2024/02/020
10.1103/PhysRevD.108.103511
10.3390/universe7110398
10.1088/1475-7516/2018/04/009
10.1088/1475-7516/2022/01/057
10.1088/1361-6382/aaa7b4
10.1103/PhysRevLett.82.2832
10.1088/1475-7516/2023/10/001
10.1103/PhysRevD.96.104046
10.1103/PhysRevD.79.123519
10.1142/S0217751X21501396
10.1103/PhysRevLett.129.041101
10.1088/1475-7516/2021/11/022
10.1103/PhysRevD.84.024028
10.1016/0550-3213(82)90037-2
10.1103/PhysRevLett.103.111303
10.1103/PhysRevD.101.083511
10.1088/1361-6633/ac1e31
10.1103/PhysRevD.105.045001
10.1088/0034-4885/58/5/001
10.1016/j.physletb.2018.01.050
10.1088/1475-7516/2023/11/020
10.1103/PhysRevLett.82.4168
10.1016/j.physletb.2005.09.070
10.1016/0370-2693(86)91126-3
10.1103/PhysRevD.73.041301
10.1088/1475-7516/2016/11/044
10.1007/JHEP07(2024)204
10.1103/PhysRevD.108.123529
10.1088/0305-4470/9/8/029
10.1103/PhysRevD.89.103501
10.1103/PhysRevD.110.115013
10.1103/PhysRevD.68.103514
10.1103/PhysRevD.108.095041
10.1016/B978-0-32-395636-9.00012-8
10.1103/RevModPhys.97.015001
10.1134/S0202289321040101
10.1103/PhysRevD.101.103508
10.1016/j.physletb.2021.136722
10.1103/PhysRevD.108.095053
10.1103/PhysRevD.54.2535
10.1103/PhysRevD.64.023508
10.1103/PhysRevD.108.023531
10.1088/1475-7516/2004/03/010
10.1103/PhysRevD.44.376
10.1103/PhysRevD.105.015023
10.1103/PhysRevD.108.124009
10.1088/1475-7516/2020/01/024
10.1103/PhysRevD.105.116011
10.1103/PhysRevD.59.102001
10.1103/PhysRevLett.126.041304
10.1016/0370-2693(81)91144-8
10.1103/PhysRevLett.102.161101
10.1103/PhysRevD.78.065048
10.1088/1475-7516/2023/10/041
10.1103/PhysRevD.106.035019
10.1103/RevModPhys.88.015004
10.1088/1475-7516/2024/01/015
10.1007/JHEP01(2019)081
10.1088/1674-4527/acdfa5
10.1103/PhysRevLett.128.031102
10.1088/1475-7516/2020/04/034
10.1103/PhysRevD.109.103001
10.1093/mnras/168.2.399
10.1103/PhysRevD.89.023512
10.1103/PhysRevD.110.063549
10.1088/1475-7516/2022/06/017
10.1103/PhysRevD.37.263
10.1103/PhysRevD.65.043514
10.1088/1475-7516/2020/10/029
10.1007/JHEP08(2023)196
10.1140/epjp/s13360-020-00564-9
10.1103/PhysRevD.102.095018
10.1103/PhysRevD.88.023516
10.1103/PhysRevLett.126.041305
10.1103/PhysRevD.109.103538
10.1103/PhysRevLett.122.201101
10.1103/PhysRevLett.128.111101
10.1103/PhysRevD.104.103021
10.1088/1475-7516/2021/12/006
10.1103/PhysRevD.43.1060
10.1088/1475-7516/2016/10/034
10.1103/PhysRevLett.72.17
10.1016/j.dark.2024.101667
10.1103/PhysRevD.107.123537
10.1088/0264-9381/23/6/004
10.1007/JHEP08(2024)060
10.1016/j.nuclphysb.2024.116528
10.1103/PhysRevD.104.075007
10.1103/PhysRevD.105.015022
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Early Universe Particle Physics
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References A Datta (25536_CR163) 2021; 127
S Datta (25536_CR52) 2021; 08
25536_CR86
K Inomata (25536_CR139) 2020; 101
25536_CR85
N Bernal (25536_CR112) 2022; 106
25536_CR82
25536_CR81
K Schmitz (25536_CR106) 2021; 01
K Saikawa (25536_CR107) 2018; 05
N Aggarwal (25536_CR145) 2021; 24
R Roshan (25536_CR35) 2025; 97
DG Figueroa (25536_CR56) 2024; 132
T Fujita (25536_CR68) 2014; 89
JD Romano (25536_CR109) 2017; 20
JJ Blanco-Pillado (25536_CR94) 2018; 778
EJ Copeland (25536_CR17) 2004; 06
25536_CR78
A Ambrosone (25536_CR133) 2022; 105
25536_CR76
25536_CR75
25536_CR74
G Lazarides (25536_CR61) 2023; 108
R Maji (25536_CR62) 2024; 01
25536_CR160
25536_CR164
WT Emond (25536_CR77) 2022; 01
DJ Reardon (25536_CR45) 2023; 951
R Samanta (25536_CR51) 2021; 05
25536_CR67
Y-P Wu (25536_CR128) 2022; 128
V Domcke (25536_CR151) 2022; 129
25536_CR66
25536_CR65
25536_CR3
A Ejlli (25536_CR152) 2019; 79
25536_CR1
J Martin (25536_CR141) 2020; 01
25536_CR2
C Caprini (25536_CR15) 2019; 11
25536_CR158
B Carr (25536_CR4) 2021; 84
M Sakellariadou (25536_CR21) 2005; 04
25536_CR157
25536_CR159
S Blasi (25536_CR49) 2021; 126
A Berlin (25536_CR153) 2022; 105
S Blasi (25536_CR91) 2020; 2
JJ Blanco-Pillado (25536_CR80) 2017; 96
25536_CR154
25536_CR55
K Schmitz (25536_CR92) 2024; 110
25536_CR54
P Di Bari (25536_CR161) 2016; 11
25536_CR53
O Lennon (25536_CR69) 2018; 04
V Domcke (25536_CR147) 2021; 126
PP Avelino (25536_CR23) 2012; 85
J Ellis (25536_CR50) 2021; 126
A Weltman (25536_CR98) 2020; 37
25536_CR146
S Antusch (25536_CR60) 2024; 10
H Xu (25536_CR46) 2023; 23
A Monin (25536_CR28) 2008; 78
MA Masoud (25536_CR32) 2021; 11
H Cheng (25536_CR93) 2024; 46
T Akutsu (25536_CR148) 2008; 101
25536_CR143
25536_CR142
25536_CR48
25536_CR47
WG Lamb (25536_CR165) 2023; 108
25536_CR44
25536_CR43
25536_CR42
25536_CR40
R Calabrese (25536_CR121) 2024; 109
N Bernal (25536_CR127) 2021; 104
D Hooper (25536_CR70) 2019; 08
D Borah (25536_CR73) 2023; 03
T Kitabayashi (25536_CR134) 2021; 36
W Buchmuller (25536_CR31) 2023; 11
G Domènech (25536_CR12) 2021; 823
P Di Bari (25536_CR162) 2020; 10
25536_CR135
25536_CR138
R-G Cai (25536_CR140) 2019; 122
25536_CR137
I Masina (25536_CR132) 2021; 27
N Bhaumik (25536_CR126) 2022; 07
G Servant (25536_CR33) 2024; 109
JJ Blanco-Pillado (25536_CR79) 2014; 89
T Papanikolaou (25536_CR10) 2021; 03
R Samanta (25536_CR72) 2022; 06
25536_CR131
25536_CR37
E Babichev (25536_CR96) 2023; 108
25536_CR119
T Hasegawa (25536_CR41) 2019; 12
R Calabrese (25536_CR124) 2023; 107
RH Cyburt (25536_CR39) 2016; 88
T Papanikolaou (25536_CR13) 2022; 10
25536_CR125
J Ellis (25536_CR57) 2024; 109
25536_CR129
A Peimbert (25536_CR95) 2016; 52
K-Y Choi (25536_CR123) 2024; 02
A Ito (25536_CR149) 2020; 80
P Auclair (25536_CR88) 2020; 101
D Matsunami (25536_CR87) 2019; 122
25536_CR120
25536_CR26
S Antusch (25536_CR38) 2024; 856
25536_CR25
D Marfatia (25536_CR63) 2024; 07
L Morrison (25536_CR71) 2019; 05
25536_CR22
25536_CR108
M Gell-Mann (25536_CR136) 1979; 790927
W Buchmuller (25536_CR30) 2021; 12
C Pallis (25536_CR64) 2024; 10
25536_CR114
25536_CR113
K Schmitz (25536_CR122) 2024; 849
L Sousa (25536_CR89) 2020; 101
R Dong (25536_CR8) 2016; 10
25536_CR118
25536_CR117
N Bernal (25536_CR130) 2021; 104
J Ellis (25536_CR24) 2023; 108
G Franciolini (25536_CR115) 2023; 108
G Domènech (25536_CR14) 2021; 7
25536_CR19
L Leblond (25536_CR27) 2009; 79
25536_CR110
25536_CR18
R Maji (25536_CR34) 2024; 08
I Esteban (25536_CR156) 2020; 09
M Sasaki (25536_CR5) 2018; 35
AD Dolgov (25536_CR7) 2011; 84
25536_CR11
MG Jackson (25536_CR20) 2005; 10
Y Cui (25536_CR90) 2019; 01
25536_CR99
S Antusch (25536_CR59) 2023; 108
B Barman (25536_CR116) 2022; 08
I Masina (25536_CR103) 2020; 135
S Balaji (25536_CR97) 2023; 10
R Anantua (25536_CR6) 2009; 103
YF Perez-Gonzalez (25536_CR111) 2021; 104
25536_CR101
N Aggarwal (25536_CR144) 2022; 128
25536_CR100
N Herman (25536_CR155) 2023; 108
25536_CR102
A Ghoshal (25536_CR36) 2023; 08
25536_CR105
25536_CR104
A Ito (25536_CR150) 2020; 80
P Auclair (25536_CR84) 2020; 04
G Dvali (25536_CR16) 2004; 03
DG Figueroa (25536_CR58) 2024; 132
L Sousa (25536_CR83) 2013; 88
A Ireland (25536_CR9) 2023; 107
W Buchmuller (25536_CR29) 2020; 811
References_xml – volume: 04
  start-page: 003
  year: 2005
  ident: 25536_CR21
  publication-title: JCAP
  doi: 10.1088/1475-7516/2005/04/003
– volume: 104
  year: 2021
  ident: 25536_CR127
  publication-title: Phys. Rev. D
  doi: 10.1103/PhysRevD.104.123536
– ident: 25536_CR67
– volume: 79
  start-page: 1032
  year: 2019
  ident: 25536_CR152
  publication-title: Eur. Phys. J. C
  doi: 10.1140/epjc/s10052-019-7542-5
– volume: 11
  start-page: 017
  year: 2019
  ident: 25536_CR15
  publication-title: JCAP
  doi: 10.1088/1475-7516/2019/11/017
– ident: 25536_CR44
– ident: 25536_CR19
  doi: 10.1103/PhysRevD.106.123515
– volume: 108
  year: 2023
  ident: 25536_CR115
  publication-title: Phys. Rev. D
  doi: 10.1103/PhysRevD.108.083527
– ident: 25536_CR143
  doi: 10.1103/PhysRevLett.87.221103
– volume: 951
  start-page: L6
  year: 2023
  ident: 25536_CR45
  publication-title: Astrophys. J. Lett.
  doi: 10.3847/2041-8213/acdd02
– ident: 25536_CR105
  doi: 10.1016/S0370-1573(99)00102-7
– ident: 25536_CR117
  doi: 10.1103/PhysRevD.107.095002
– volume: 03
  start-page: 053
  year: 2021
  ident: 25536_CR10
  publication-title: JCAP
  doi: 10.1088/1475-7516/2021/03/053
– volume: 849
  year: 2024
  ident: 25536_CR122
  publication-title: Phys. Lett. B
  doi: 10.1016/j.physletb.2024.138473
– ident: 25536_CR99
– volume: 101
  year: 2008
  ident: 25536_CR148
  publication-title: Phys. Rev. Lett.
  doi: 10.1103/PhysRevLett.101.101101
– volume: 01
  start-page: 097
  year: 2021
  ident: 25536_CR106
  publication-title: JHEP
  doi: 10.1007/JHEP01(2021)097
– volume: 85
  year: 2012
  ident: 25536_CR23
  publication-title: Phys. Rev. D
  doi: 10.1103/PhysRevD.85.083525
– volume: 132
  year: 2024
  ident: 25536_CR56
  publication-title: Phys. Rev. Lett.
  doi: 10.1103/PhysRevLett.132.171002
– ident: 25536_CR142
– ident: 25536_CR146
  doi: 10.1103/PhysRevD.95.063002
– ident: 25536_CR1
  doi: 10.1093/mnras/152.1.75
– volume: 07
  start-page: 130
  year: 2022
  ident: 25536_CR126
  publication-title: JHEP
  doi: 10.1007/JHEP07(2022)130
– volume: 109
  year: 2024
  ident: 25536_CR57
  publication-title: Phys. Rev. D
  doi: 10.1103/PhysRevD.109.023522
– volume: 24
  start-page: 4
  year: 2021
  ident: 25536_CR145
  publication-title: Living Rev. Rel.
  doi: 10.1007/s41114-021-00032-5
– volume: 12
  start-page: 012
  year: 2019
  ident: 25536_CR41
  publication-title: JCAP
  doi: 10.1088/1475-7516/2019/12/012
– volume: 10
  start-page: 013
  year: 2005
  ident: 25536_CR20
  publication-title: JHEP
  doi: 10.1088/1126-6708/2005/10/013
– ident: 25536_CR75
  doi: 10.1103/PhysRevD.31.3052
– ident: 25536_CR85
  doi: 10.1103/PhysRevD.64.064008
– volume: 80
  start-page: 179
  year: 2020
  ident: 25536_CR149
  publication-title: Eur. Phys. J. C
  doi: 10.1140/epjc/s10052-020-7735-y
– volume: 05
  start-page: 211
  year: 2021
  ident: 25536_CR51
  publication-title: JHEP
  doi: 10.1007/JHEP05(2021)211
– ident: 25536_CR47
– ident: 25536_CR26
  doi: 10.1103/PhysRevD.47.2324
– volume: 122
  year: 2019
  ident: 25536_CR87
  publication-title: Phys. Rev. Lett.
  doi: 10.1103/PhysRevLett.122.201301
– volume: 10
  start-page: 211
  year: 2024
  ident: 25536_CR64
  publication-title: Universe
  doi: 10.3390/universe10050211
– volume: 09
  start-page: 178
  year: 2020
  ident: 25536_CR156
  publication-title: JHEP
  doi: 10.1007/JHEP09(2020)178
– volume: 127
  year: 2021
  ident: 25536_CR163
  publication-title: Phys. Rev. Lett.
  doi: 10.1103/PhysRevLett.127.231801
– volume: 05
  start-page: 005
  year: 2019
  ident: 25536_CR71
  publication-title: JCAP
  doi: 10.1088/1475-7516/2019/05/005
– volume: 107
  year: 2023
  ident: 25536_CR9
  publication-title: Phys. Rev. D
  doi: 10.1103/PhysRevD.107.104021
– ident: 25536_CR66
  doi: 10.1088/0264-9381/32/7/074001
– ident: 25536_CR11
  doi: 10.1088/1475-7516/2021/04/062
– volume: 811
  year: 2020
  ident: 25536_CR29
  publication-title: Phys. Lett. B
  doi: 10.1016/j.physletb.2020.135914
– volume: 856
  year: 2024
  ident: 25536_CR38
  publication-title: Phys. Lett. B
  doi: 10.1016/j.physletb.2024.138924
– ident: 25536_CR65
– volume: 03
  start-page: 127
  year: 2023
  ident: 25536_CR73
  publication-title: JHEP
  doi: 10.1007/JHEP03(2023)127
– volume: 08
  start-page: 001
  year: 2019
  ident: 25536_CR70
  publication-title: JHEP
  doi: 10.1007/JHEP08(2019)001
– ident: 25536_CR18
  doi: 10.1016/j.physletb.2023.137724
– volume: 08
  start-page: 068
  year: 2022
  ident: 25536_CR116
  publication-title: JCAP
  doi: 10.1088/1475-7516/2022/08/068
– volume: 101
  year: 2020
  ident: 25536_CR139
  publication-title: Phys. Rev. D
  doi: 10.1103/PhysRevD.101.123533
– ident: 25536_CR154
– ident: 25536_CR110
  doi: 10.1103/PhysRevD.73.064006
– ident: 25536_CR42
– volume: 20
  start-page: 2
  year: 2017
  ident: 25536_CR109
  publication-title: Living Rev. Rel.
  doi: 10.1007/s41114-017-0004-1
– ident: 25536_CR119
  doi: 10.1103/PhysRevD.110.043528
– volume: 10
  start-page: 089
  year: 2022
  ident: 25536_CR13
  publication-title: JCAP
  doi: 10.1088/1475-7516/2022/10/089
– volume: 06
  start-page: 013
  year: 2004
  ident: 25536_CR17
  publication-title: JHEP
  doi: 10.1088/1126-6708/2004/06/013
– volume: 80
  start-page: 545
  year: 2020
  ident: 25536_CR150
  publication-title: Eur. Phys. J. C
  doi: 10.1140/epjc/s10052-020-8092-6
– volume: 08
  start-page: 021
  year: 2021
  ident: 25536_CR52
  publication-title: JCAP
  doi: 10.1088/1475-7516/2021/08/021
– ident: 25536_CR78
– ident: 25536_CR129
  doi: 10.1103/PhysRevD.104.083523
– volume: 37
  year: 2020
  ident: 25536_CR98
  publication-title: Publ. Astron. Soc. Austral.
  doi: 10.1017/pasa.2019.42
– volume: 126
  year: 2021
  ident: 25536_CR147
  publication-title: Phys. Rev. Lett.
  doi: 10.1103/PhysRevLett.126.021104
– volume: 10
  start-page: 007
  year: 2024
  ident: 25536_CR60
  publication-title: JCAP
  doi: 10.1088/1475-7516/2024/10/007
– volume: 108
  year: 2023
  ident: 25536_CR165
  publication-title: Phys. Rev. D
  doi: 10.1103/PhysRevD.108.103019
– volume: 2
  year: 2020
  ident: 25536_CR91
  publication-title: Phys. Rev. Res.
  doi: 10.1103/PhysRevResearch.2.043321
– volume: 05
  start-page: 035
  year: 2018
  ident: 25536_CR107
  publication-title: JCAP
  doi: 10.1088/1475-7516/2018/05/035
– volume: 02
  start-page: 020
  year: 2024
  ident: 25536_CR123
  publication-title: JCAP
  doi: 10.1088/1475-7516/2024/02/020
– volume: 108
  year: 2023
  ident: 25536_CR24
  publication-title: Phys. Rev. D
  doi: 10.1103/PhysRevD.108.103511
– volume: 7
  start-page: 398
  year: 2021
  ident: 25536_CR14
  publication-title: Universe
  doi: 10.3390/universe7110398
– volume: 04
  start-page: 009
  year: 2018
  ident: 25536_CR69
  publication-title: JCAP
  doi: 10.1088/1475-7516/2018/04/009
– volume: 01
  start-page: 057
  year: 2022
  ident: 25536_CR77
  publication-title: JCAP
  doi: 10.1088/1475-7516/2022/01/057
– volume: 35
  year: 2018
  ident: 25536_CR5
  publication-title: Class. Quant. Grav.
  doi: 10.1088/1361-6382/aaa7b4
– ident: 25536_CR160
  doi: 10.1103/PhysRevLett.82.2832
– ident: 25536_CR101
– ident: 25536_CR125
  doi: 10.1088/1475-7516/2023/10/001
– volume: 96
  year: 2017
  ident: 25536_CR80
  publication-title: Phys. Rev. D
  doi: 10.1103/PhysRevD.96.104046
– volume: 79
  year: 2009
  ident: 25536_CR27
  publication-title: Phys. Rev. D
  doi: 10.1103/PhysRevD.79.123519
– volume: 36
  start-page: 2150139
  year: 2021
  ident: 25536_CR134
  publication-title: Int. J. Mod. Phys. A
  doi: 10.1142/S0217751X21501396
– volume: 129
  year: 2022
  ident: 25536_CR151
  publication-title: Phys. Rev. Lett.
  doi: 10.1103/PhysRevLett.129.041101
– volume: 11
  start-page: 022
  year: 2021
  ident: 25536_CR32
  publication-title: JCAP
  doi: 10.1088/1475-7516/2021/11/022
– volume: 84
  year: 2011
  ident: 25536_CR7
  publication-title: Phys. Rev. D
  doi: 10.1103/PhysRevD.84.024028
– ident: 25536_CR25
  doi: 10.1016/0550-3213(82)90037-2
– volume: 103
  year: 2009
  ident: 25536_CR6
  publication-title: Phys. Rev. Lett.
  doi: 10.1103/PhysRevLett.103.111303
– volume: 101
  year: 2020
  ident: 25536_CR88
  publication-title: Phys. Rev. D
  doi: 10.1103/PhysRevD.101.083511
– volume: 84
  year: 2021
  ident: 25536_CR4
  publication-title: Rept. Prog. Phys.
  doi: 10.1088/1361-6633/ac1e31
– volume: 105
  year: 2022
  ident: 25536_CR133
  publication-title: Phys. Rev. D
  doi: 10.1103/PhysRevD.105.045001
– ident: 25536_CR54
  doi: 10.1088/0034-4885/58/5/001
– volume: 778
  start-page: 392
  year: 2018
  ident: 25536_CR94
  publication-title: Phys. Lett. B
  doi: 10.1016/j.physletb.2018.01.050
– ident: 25536_CR48
– volume: 11
  start-page: 020
  year: 2023
  ident: 25536_CR31
  publication-title: JCAP
  doi: 10.1088/1475-7516/2023/11/020
– ident: 25536_CR40
  doi: 10.1103/PhysRevLett.82.4168
– ident: 25536_CR157
  doi: 10.1016/j.physletb.2005.09.070
– ident: 25536_CR100
– ident: 25536_CR137
  doi: 10.1016/0370-2693(86)91126-3
– ident: 25536_CR22
  doi: 10.1103/PhysRevD.73.041301
– volume: 11
  start-page: 044
  year: 2016
  ident: 25536_CR161
  publication-title: JCAP
  doi: 10.1088/1475-7516/2016/11/044
– volume: 07
  start-page: 204
  year: 2024
  ident: 25536_CR63
  publication-title: JHEP
  doi: 10.1007/JHEP07(2024)204
– volume: 108
  year: 2023
  ident: 25536_CR96
  publication-title: Phys. Rev. D
  doi: 10.1103/PhysRevD.108.123529
– ident: 25536_CR53
  doi: 10.1088/0305-4470/9/8/029
– volume: 89
  year: 2014
  ident: 25536_CR68
  publication-title: Phys. Rev. D
  doi: 10.1103/PhysRevD.89.103501
– ident: 25536_CR120
  doi: 10.1103/PhysRevD.110.115013
– ident: 25536_CR55
  doi: 10.1103/PhysRevD.68.103514
– volume: 108
  year: 2023
  ident: 25536_CR61
  publication-title: Phys. Rev. D
  doi: 10.1103/PhysRevD.108.095041
– ident: 25536_CR3
  doi: 10.1016/B978-0-32-395636-9.00012-8
– volume: 97
  year: 2025
  ident: 25536_CR35
  publication-title: Rev. Mod. Phys.
  doi: 10.1103/RevModPhys.97.015001
– volume: 27
  start-page: 315
  year: 2021
  ident: 25536_CR132
  publication-title: Grav. Cosmol.
  doi: 10.1134/S0202289321040101
– volume: 101
  year: 2020
  ident: 25536_CR89
  publication-title: Phys. Rev. D
  doi: 10.1103/PhysRevD.101.103508
– volume: 52
  start-page: 419
  year: 2016
  ident: 25536_CR95
  publication-title: Rev. Mex. Astron. Astrofis.
– volume: 823
  year: 2021
  ident: 25536_CR12
  publication-title: Phys. Lett. B
  doi: 10.1016/j.physletb.2021.136722
– ident: 25536_CR43
– volume: 108
  year: 2023
  ident: 25536_CR59
  publication-title: Phys. Rev. D
  doi: 10.1103/PhysRevD.108.095053
– ident: 25536_CR81
  doi: 10.1103/PhysRevD.54.2535
– ident: 25536_CR102
  doi: 10.1103/PhysRevD.64.023508
– ident: 25536_CR37
  doi: 10.1103/PhysRevD.108.023531
– volume: 03
  start-page: 010
  year: 2004
  ident: 25536_CR16
  publication-title: JCAP
  doi: 10.1088/1475-7516/2004/03/010
– ident: 25536_CR104
  doi: 10.1103/PhysRevD.44.376
– ident: 25536_CR113
  doi: 10.1103/PhysRevD.105.015023
– volume: 108
  year: 2023
  ident: 25536_CR155
  publication-title: Phys. Rev. D
  doi: 10.1103/PhysRevD.108.124009
– volume: 01
  start-page: 024
  year: 2020
  ident: 25536_CR141
  publication-title: JCAP
  doi: 10.1088/1475-7516/2020/01/024
– volume: 105
  year: 2022
  ident: 25536_CR153
  publication-title: Phys. Rev. D
  doi: 10.1103/PhysRevD.105.116011
– ident: 25536_CR108
  doi: 10.1103/PhysRevD.59.102001
– volume: 126
  year: 2021
  ident: 25536_CR50
  publication-title: Phys. Rev. Lett.
  doi: 10.1103/PhysRevLett.126.041304
– ident: 25536_CR74
  doi: 10.1016/0370-2693(81)91144-8
– ident: 25536_CR138
  doi: 10.1103/PhysRevLett.102.161101
– volume: 790927
  start-page: 315
  year: 1979
  ident: 25536_CR136
  publication-title: Conf. Proc. C
– volume: 78
  year: 2008
  ident: 25536_CR28
  publication-title: Phys. Rev. D
  doi: 10.1103/PhysRevD.78.065048
– volume: 10
  start-page: 041
  year: 2023
  ident: 25536_CR97
  publication-title: JCAP
  doi: 10.1088/1475-7516/2023/10/041
– volume: 106
  year: 2022
  ident: 25536_CR112
  publication-title: Phys. Rev. D
  doi: 10.1103/PhysRevD.106.035019
– volume: 88
  year: 2016
  ident: 25536_CR39
  publication-title: Rev. Mod. Phys.
  doi: 10.1103/RevModPhys.88.015004
– volume: 01
  start-page: 015
  year: 2024
  ident: 25536_CR62
  publication-title: JCAP
  doi: 10.1088/1475-7516/2024/01/015
– volume: 01
  start-page: 081
  year: 2019
  ident: 25536_CR90
  publication-title: JHEP
  doi: 10.1007/JHEP01(2019)081
– volume: 23
  year: 2023
  ident: 25536_CR46
  publication-title: Res. Astron. Astrophys.
  doi: 10.1088/1674-4527/acdfa5
– volume: 128
  year: 2022
  ident: 25536_CR128
  publication-title: Phys. Rev. Lett.
  doi: 10.1103/PhysRevLett.128.031102
– volume: 04
  start-page: 034
  year: 2020
  ident: 25536_CR84
  publication-title: JCAP
  doi: 10.1088/1475-7516/2020/04/034
– volume: 109
  year: 2024
  ident: 25536_CR121
  publication-title: Phys. Rev. D
  doi: 10.1103/PhysRevD.109.103001
– ident: 25536_CR2
  doi: 10.1093/mnras/168.2.399
– volume: 89
  year: 2014
  ident: 25536_CR79
  publication-title: Phys. Rev. D
  doi: 10.1103/PhysRevD.89.023512
– volume: 110
  year: 2024
  ident: 25536_CR92
  publication-title: Phys. Rev. D
  doi: 10.1103/PhysRevD.110.063549
– volume: 06
  start-page: 017
  year: 2022
  ident: 25536_CR72
  publication-title: JCAP
  doi: 10.1088/1475-7516/2022/06/017
– ident: 25536_CR76
  doi: 10.1103/PhysRevD.37.263
– ident: 25536_CR82
  doi: 10.1103/PhysRevD.65.043514
– volume: 132
  year: 2024
  ident: 25536_CR58
  publication-title: Phys. Rev. Lett.
  doi: 10.1103/PhysRevLett.132.171002
– volume: 10
  start-page: 029
  year: 2020
  ident: 25536_CR162
  publication-title: JCAP
  doi: 10.1088/1475-7516/2020/10/029
– volume: 08
  start-page: 196
  year: 2023
  ident: 25536_CR36
  publication-title: JHEP
  doi: 10.1007/JHEP08(2023)196
– volume: 135
  start-page: 552
  year: 2020
  ident: 25536_CR103
  publication-title: Eur. Phys. J. Plus
  doi: 10.1140/epjp/s13360-020-00564-9
– ident: 25536_CR114
  doi: 10.1103/PhysRevD.102.095018
– volume: 88
  year: 2013
  ident: 25536_CR83
  publication-title: Phys. Rev. D
  doi: 10.1103/PhysRevD.88.023516
– volume: 126
  year: 2021
  ident: 25536_CR49
  publication-title: Phys. Rev. Lett.
  doi: 10.1103/PhysRevLett.126.041305
– volume: 109
  year: 2024
  ident: 25536_CR33
  publication-title: Phys. Rev. D
  doi: 10.1103/PhysRevD.109.103538
– volume: 122
  year: 2019
  ident: 25536_CR140
  publication-title: Phys. Rev. Lett.
  doi: 10.1103/PhysRevLett.122.201101
– volume: 128
  year: 2022
  ident: 25536_CR144
  publication-title: Phys. Rev. Lett.
  doi: 10.1103/PhysRevLett.128.111101
– ident: 25536_CR158
  doi: 10.1016/j.physletb.2005.09.070
– volume: 104
  year: 2021
  ident: 25536_CR111
  publication-title: Phys. Rev. D
  doi: 10.1103/PhysRevD.104.103021
– volume: 12
  start-page: 006
  year: 2021
  ident: 25536_CR30
  publication-title: JCAP
  doi: 10.1088/1475-7516/2021/12/006
– ident: 25536_CR86
  doi: 10.1103/PhysRevD.43.1060
– volume: 10
  start-page: 034
  year: 2016
  ident: 25536_CR8
  publication-title: JCAP
  doi: 10.1088/1475-7516/2016/10/034
– ident: 25536_CR159
  doi: 10.1103/PhysRevLett.72.17
– volume: 46
  year: 2024
  ident: 25536_CR93
  publication-title: Phys. Dark Univ.
  doi: 10.1016/j.dark.2024.101667
– volume: 107
  year: 2023
  ident: 25536_CR124
  publication-title: Phys. Rev. D
  doi: 10.1103/PhysRevD.107.123537
– ident: 25536_CR135
  doi: 10.1088/0264-9381/23/6/004
– ident: 25536_CR164
– volume: 08
  start-page: 060
  year: 2024
  ident: 25536_CR34
  publication-title: JHEP
  doi: 10.1007/JHEP08(2024)060
– ident: 25536_CR118
  doi: 10.1016/j.nuclphysb.2024.116528
– volume: 104
  year: 2021
  ident: 25536_CR130
  publication-title: Phys. Rev. D
  doi: 10.1103/PhysRevD.104.075007
– ident: 25536_CR131
  doi: 10.1103/PhysRevD.105.015022
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Snippet A bstract While topologically stable cosmic strings are disfavoured by the recent observation of nHz stochastic gravitational waves (GW) by Pulsar Timing...
While topologically stable cosmic strings are disfavoured by the recent observation of nHz stochastic gravitational waves (GW) by Pulsar Timing Arrays (PTA),...
Abstract While topologically stable cosmic strings are disfavoured by the recent observation of nHz stochastic gravitational waves (GW) by Pulsar Timing Arrays...
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SubjectTerms Baryo-and Leptogenesis
Black Holes
Classical and Quantum Gravitation
Cosmology of Theories BSM
Early Universe Particle Physics
Elementary Particles
Gravitational waves
Hawking radiation
High energy physics
LIGO (observatory)
Physics
Physics and Astronomy
Pulsars
Quantum Field Theories
Quantum Field Theory
Quantum Physics
Regular Article - Theoretical Physics
Relativity Theory
String Theory
Universe
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Title Cosmic superstrings, metastable strings and ultralight primordial black holes: from NANOGrav to LIGO and beyond
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