REVIEW 3 minor 124 references
Constraints on New Physics from $B$ mesons
T0 review · 0 major / 3 minor · reviewed 2026-08-14 · deepseek-v4-flash
Pith's one-line read Persistent anomalies in B-meson decays and mixing may be the first indirect signs of new physics.
desk verdict A solid, honest proceedings review that makes no new claims but accurately maps the 2019 B-decay anomaly landscape; worth a referee's time only to check accuracy. read the letter →
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
The reading
What carries the argument
The central objects are flavour-changing neutral current (FCNC) transitions, which are loop-, CKM-, and GIM-suppressed in the Standard Model and therefore intrinsically sensitive to small new-physics effects. The argument is carried by a set of normalised observables: the lepton-flavour-universality ratios $R(D^{(*)})$ and $R_{K^{(*)}}$, the ratio $\Delta M_d/\Delta M_s$ of neutral $B$-meson mass differences, and the direct-CP-violation parameter $\varepsilon'/\varepsilon$ in $K\to\pi\pi$. Model-independently, new physics is parametrised by effective Hamiltonians with Wilson coefficients such as $C_9^{bs\mu\mu}$, $C_{10}^{bs\mu\mu}$, and the $b\to c\tau\nu$ coefficients $C_V^L$, $C_S^L$, $C_S^R$, $C_T$. For the mixing tension, the load-bearing comparison is between the tree-level measurement of $\gamma$ from $B\to DK$ and the indirect value obtained from $\Delta M_d/\Delta M_s$ together with the lattice QCD ratio $\xi$ of hadronic matrix elements; the author uses this machinery to argue that the resulting pattern would require flavour-non-universal new physics in $\Delta F=2$ transitions, with larger effects in $b\to d$ than in $b\to s$.
What would settle it
A more precise measurement of $\gamma$ from $B\to DK$ at LHCb and Belle II, combined with an independent lattice-QCD determination of $\xi$, would settle the mixing question: if $\gamma$ moves down toward $(63.0\pm2.1)^\circ$ with reduced uncertainty, the new-physics interpretation is supported, whereas if $\gamma$ stays near $74^\circ$ while the lattice average shifts to the HPQCD value, the anomaly vanishes. For $\varepsilon'/\varepsilon$, an improved lattice calculation of the $K\to\pi\pi$ hadronic matrix elements that brings the Standard Model prediction up to $(16.6\pm2.3)\times10^{-4}$ would remove that anomaly; a NA62 or KOTO measurement of $K\to\pi\nu\bar\nu$ at the Standard Model rate would likewise disfavour the new-physics interpretation.
Extended reading notes
Core claim
The paper's central assessment is that the observed anomalies in charged and neutral current $B$ decays, together with tensions in $\Delta M_d/\Delta M_s$ and $\varepsilon'/\varepsilon$, may be first signs of new physics. For neutral $B$ mixing, using the Fermilab/MILC lattice value of the hadronic ratio $\xi$ to convert $\Delta M_d/\Delta M_s$ into an indirect determination of $\gamma$ yields $\gamma=(63.0\pm 2.1)^\circ$, nearly $2\sigma$ below the LHCb measurement $\gamma=(74.0^{+5.0}_{-5.8})^\circ$; the author states that if future measurements confirm this, it 'would unambiguously imply the presence of NP in $\Delta M_d$ and/or $\Delta M_s$.' She also stresses that this anomaly is not unambiguous, because the HPQCD lattice results show no deviation. In the $b\to c\tau\nu$ sector, $R(D^{(*)})$ sits $3.1\sigma$ above the Standard Model, and in $b\to s\ell^+\ell^-$ global fits a non-zero $C_9^{bs\mu\mu}\simeq -0.97$ or $C_9^{bs\mu\mu}=-C_{10}^{bs\mu\mu}\simeq -0.53$ is preferred at about $6\sigma$. The paper further records a $2.9\sigma$ gap between the measured $\varepsilon'/\varepsilon$ and the recent lattice-based Standard Model prediction.
Load-bearing premise
The load-bearing premise is that the Fermilab/MILC lattice calculation of $\xi$, the ratio of hadronic matrix elements entering $B_d$ and $B_s$ mixing, is the correct input for converting $\Delta M_d/\Delta M_s$ into $\gamma$; if the competing HPQCD value is right instead, the tension disappears and the case for new physics in $B$ mixing collapses.
Editorial extensions
If this is right
- If the $\Delta M_d/\Delta M_s$ tension is confirmed by more accurate determinations of $\gamma$, new physics must modify $\Delta F=2$ transitions with larger effects in $b\to d$ than in $b\to s$, which cannot be accommodated by constrained minimal flavour violation or minimally broken $U(2)^3$ symmetry.
- The $R(D^{(*)})$ and $R_{K^{(*)}}$ anomalies can be jointly explained by an $SU(2)_L$-singlet vector leptoquark, which arises naturally from Pati-Salam unification and is least constrained by complementary observables such as $B_s-\bar B_s$ mixing and $B\to K^{(*)}\nu\bar\nu$.
- Global fits to $b\to s\ell^+\ell^-$ data single out $C_9^{bs\mu\mu}\simeq -0.97$ (or $C_9^{bs\mu\mu}=-C_{10}^{bs\mu\mu}\simeq -0.53$) with about $6\sigma$ pull relative to the Standard Model, and a non-zero $C_{10}^{bs\mu\mu}$ is needed to accommodate the suppression of $B_s\to\mu^+\mu^-$.
- Rare kaon decays $K\to\pi\nu\bar\nu$ can probe new physics at scales beyond $100$ TeV, and a new-physics contribution to $\varepsilon'/\varepsilon$ is generally correlated with a deviation in $\mathrm{BR}(K_L\to\pi^0\nu\bar\nu)$ from its Standard Model prediction.
- None of the currently considered simplified models fully resolves all anomalies: the charged Higgs scalar gives the best fit to $b\to c\tau\nu$ data but predicts $\mathrm{BR}(B_c\to\tau\nu)>50\%$ and sits in tension with mono-$\tau$ searches.
Reading between the lines
- One testable extension the review leaves implicit: if the $\Delta M_d$ anomaly reflects a new CP-violating phase of about $\pi/2$ in the $b\to d$ transition, the same phase should generate enhanced CP asymmetries in $b\to d$ penguin-influenced decays such as $B_d\to\pi\pi$; Belle II and LHCb data on these decays could corroborate the mixing signal.
- Because the $SU(2)_L$-singlet vector leptoquark that fits $R(D^{(*)})$ and $R_{K^{(*)}}$ has TeV-scale mass and flavour non-universal couplings, it also predicts lepton-flavour-violating decays such as $B\to K\tau\mu$; the review notes the related constraints from $K_L\to\mu e$ but does not list $B\to K\tau\mu$ as a headline signature worth searching for.
- The CKM-hierarchy argument that makes kaon FCNCs the most sensitive probes implies an experimental prioritisation the author does not state: if new physics is to be discovered through flavour, the highest-yield searches may be $K_L\to\pi^0\nu\bar\nu$ and $K^+\to\pi^+\nu\bar\nu$ at KOTO and NA62, rather than further $B$-decay asymmetry measurements.
- If the $\varepsilon'/\varepsilon$ anomaly and the $K\to\pi\nu\bar\nu$ rates both stay at their Standard Model values while lattice QCD improves, the logical conclusion would be that the current $2.9\sigma$ gap is a hadronic-matrix-element artefact; this is a possible outcome of the review's own logic but not one it emphasises.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. This is a conference proceedings review by Monika Blanke, based on a talk at LeptonPhoton 2019, summarizing the status of New Physics in flavour-violating B decays. The paper reviews three main areas: (i) neutral B meson mixing, where a roughly 2 sigma tension is reported between the tree-level CKM determination of gamma and the ratio Delta M_d/Delta M_s, a tension that is explicitly flagged as not unambiguous because it depends on the lattice value of xi and disappears with the HPQCD determination; (ii) the charged-current b to c tau nu anomalies in R(D^(*)) and related observables, with a survey of simplified NP models and their tensions; and (iii) the neutral-current b to s l+ l- anomalies, including global-fit pulls and popular leptoquark or Z' explanations. The final section advocates kaon physics, discussing epsilon'/epsilon and K to pi nu nu bar as probes of very high scales. The paper makes no new quantitative claim and its conclusions are explicitly conditional on future measurements and improved lattice inputs.
Significance. As a proceedings review, the paper's value lies in its compact, balanced, and well-referenced status report of active anomalies in flavour physics. It usefully collects the relevant global-fit results, lattice inputs, and simplified-model constraints, and it explicitly flags the fragility of the Delta M_d/Delta M_s tension and the epsilon'/epsilon tension. The central conditional claim, that confirmation of the gamma discrepancy together with the Fermilab/MILC lattice value of xi would unambiguously require NP in Delta M_d and/or Delta M_s, is internally sound given its stated assumptions. The review also credits and cross-checks the author's own work against independent lattice determinations by Fermilab/MILC, RBC/UKQCD, HPQCD, and QCD sum rules. The significance is moderate but appropriate for the venue: a useful, honest snapshot rather than a new quantitative result.
minor comments (3)
- [Section 2] The sentence 'Using instead the values of xi found by RBC/UKQCD [11], HPQCD [12], or QCD sum rules [13-17] yields similar results' is difficult to reconcile with the later statement in the same section that the HPQCD results [12] 'show no deviation from the data in either Delta M_d or Delta M_s.' Please rephrase to attribute the 'similar results' statement to RBC/UKQCD and the sum-rule determinations and to state explicitly that HPQCD is the outlier; as written, the two sentences are contradictory.
- [References] Reference [75] (Kowalska, Kumar, Sessolo) does not appear to be cited in the body text; either add a citation at the appropriate place in Section 4 or remove the entry from the bibliography.
- [Section 5] In the sentence 'Interestingly the presence of an anomaly is supported by dual QCD calculations [105, 112]; however it is not seen with the use of chiral perturbation theory methods [113]', the phrase 'it is not seen' is slightly ambiguous about whether the tension or the anomaly is not seen; consider rephrasing to state explicitly that the chiral perturbation theory analysis does not find a deviation from the Standard Model prediction.
Circularity Check
No significant circularity: the review is a survey of external data and independent fits; self-citations are traceable to published analyses with external inputs and are not load-bearing.
full rationale
This proceedings article makes no new quantitative claim; its content is a report on external experimental results (LHCb, Belle, BaBar, ATLAS, CMS) and on global fits and lattice calculations by independent groups. The strongest statements are conditional: Section 2 quotes a 2sigma tension between tree-level gamma and the indirect determination from DeltaM_d/DeltaM_s using the Fermilab/MILC value of xi, and states that 'This tension, if confirmed by future more accurate determinations of gamma, would unambiguously imply the presence of NP in DeltaM_d and/or DeltaM_s.' The input xi is external lattice data, and the review explicitly flags the anomaly as 'not unambiguous' because HPQCD [12] sees no deviation and QCD sum rules [17] are compatible with both. The R(D(*)) and b->s l+l- sections report fits by external groups [49] and model scenarios from published papers; the R(Lambda_c) sum-rule prediction in Eq. (3.3) is a model-independent relation applied to external measurements, not a parameter fitted from the predicted observable. The epsilon'/epsilon discussion cites independent lattice and dual-QCD calculations with the experimental value, and notes the chiral perturbation theory countervailing result. Self-citations to the author's own works [7,10,26,38,39,101] are present, but they point to published EPJC/PRD/PRL analyses whose inputs are external experimental and lattice data; none of these citations is used to define away an independent test or to import an unverified uniqueness claim. The review's own caveats identify the load-bearing uncertainties (notably xi and the lattice determination of K->pi pi matrix elements) rather than hiding them. The derivation chain therefore does not reduce to its inputs by construction.
Assumptions & free parameters
assumptions (2)
- domain assumption The Standard Model effective Hamiltonian describes the relevant b to s, b to c, and s to d transitions.
- domain assumption The CKM matrix is described by four real parameters, and tree-level determinations of gamma, Vub, and Vcb are free of new physics contamination.
Cite this review
Pith. "Pith review of Constraints on New Physics from $B$ mesons." pith.science (2026). https://pith.science/paper/5OTKK6AH
@misc{pith2026190809713,
author = {Pith},
title = {Pith review of: Constraints on New Physics from $B$ mesons},
year = {2026},
howpublished = {\url{https://pith.science/paper/5OTKK6AH}},
note = {Machine review of arXiv:1908.09713}
}
abstract
These proceedings review the status of New Physics contributions to flavour violating $B$ decays. The anomalies in charged and neutral current $B$ decays related to lepton flavour universality violation have received a substantial amount of attention over the past years, and we discuss the current status in light of the new data presented earlier this year. We also recall a tension in the neutral $B$ meson mixing observables $\Delta M_d$ and $\Delta M_s$ and in particular their ratio, when compared with their SM predictions obtained using tree-level determinations of the CKM matrix and the recent lattice QCD results for the relevant hadronic matrix elements. Last but not least, we advocate kaon physics as a unique probe of very high energy scales and briefly discuss the current status of $\varepsilon'/\varepsilon$ and $K\to\pi\nu\bar\nu$.
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Works this paper leans on
- [1]
-
[2]
P. Gambino, M. Jung and S. Schacht, Phys. Lett. B 795 (2019) 386 [arXiv:1905.08209 [hep-ph]]
arXiv 2019
-
[3]
LHCb Collaboration, M. W. Kenzie and M. P. Whitehead, LHCb-CONF-2018-002
2018
- [4]
- [5]
- [6]
-
[7]
M. Blanke and A. J. Buras, Eur. Phys. J. C 79 (2019) no.2, 159 [arXiv:1812.06963 [hep-ph]]
arXiv 2019
-
[8]
Y . Amhis et al. [HFLA V Collaboration], Eur. Phys. J. C77 (2017) no.12, 895 [arXiv:1612.07233 [hep-ex]]. Updates available at https://hflav.web.cern.ch/
arXiv 2017
Show all 124 references
-
[9]
Bazavov et al
A. Bazavov et al. [Fermilab Lattice and MILC Collaborations], Phys. Rev. D 93 (2016) no.11, 113016 [arXiv:1602.03560 [hep-lat]]
2016 arXiv
-
[10]
Blanke and A
M. Blanke and A. J. Buras, Eur. Phys. J. C 76 (2016) no.4, 197 [arXiv:1602.04020 [hep-ph]]
2016 arXiv
-
[11]
P. A. Boyle et al. [RBC/UKQCD Collaboration], arXiv:1812.08791 [hep-lat]
-
[12]
R. J. Dowdall, C. T. H. Davies, R. R. Horgan, G. P. Lepage, C. J. Monahan, J. Shigemitsu and M. Wingate, arXiv:1907.01025 [hep-lat]
1907 arXiv
-
[13]
A. G. Grozin, R. Klein, T. Mannel and A. A. Pivovarov, Phys. Rev. D 94 (2016) no.3, 034024 [arXiv:1606.06054 [hep-ph]]
2016 arXiv
-
[14]
A. G. Grozin, T. Mannel and A. A. Pivovarov, Phys. Rev. D 96 (2017) no.7, 074032 [arXiv:1706.05910 [hep-ph]]. 9 Constraints on New Physics from B mesons Monika Blanke
2017 arXiv
-
[15]
M. Kirk, A. Lenz and T. Rauh, JHEP 1712 (2017) 068 [arXiv:1711.02100 [hep-ph]]
2017 arXiv
-
[16]
A. G. Grozin, T. Mannel and A. A. Pivovarov, Phys. Rev. D 98 (2018) no.5, 054020 [arXiv:1806.00253 [hep-ph]]
2018 arXiv
-
[17]
D. King, A. Lenz and T. Rauh, JHEP 1905 (2019) 034 [arXiv:1904.00940 [hep-ph]]
2019 arXiv
- [18]
-
[19]
A. J. Buras, P. Gambino, M. Gorbahn, S. Jager and L. Silvestrini, Phys. Lett. B 500 (2001) 161 [hep-ph/0007085]
2001 arXiv
-
[20]
A. J. Buras, Acta Phys. Polon. B 34 (2003) 5615 [hep-ph/0310208]
2003 arXiv
-
[21]
Blanke, A
M. Blanke, A. J. Buras, D. Guadagnoli and C. Tarantino, JHEP 0610 (2006) 003 [hep-ph/0604057]
2006 arXiv
-
[22]
A. L. Kagan, G. Perez, T. V olansky and J. Zupan, Phys. Rev. D80 (2009) 076002 [arXiv:0903.1794 [hep-ph]]
2009 arXiv
-
[23]
Barbieri, G
R. Barbieri, G. Isidori, J. Jones-Perez, P. Lodone and D. M. Straub, Eur. Phys. J. C 71 (2011) 1725 [arXiv:1105.2296 [hep-ph]]
2011 arXiv
-
[24]
Barbieri, D
R. Barbieri, D. Buttazzo, F. Sala and D. M. Straub, JHEP 1207 (2012) 181 [arXiv:1203.4218 [hep-ph]]
2012 arXiv
-
[25]
A. J. Buras and J. Girrbach, JHEP 1301 (2013) 007 [arXiv:1206.3878 [hep-ph]]
2013 arXiv
-
[26]
Blanke, Acta Phys
M. Blanke, Acta Phys. Polon. B 41 (2010) 127 [arXiv:0904.2528 [hep-ph]]
2010 arXiv
-
[27]
J. A. Bailey, S. Lee, W. Lee, J. Leem and S. Park, Phys. Rev. D 98 (2018) no.9, 094505 [arXiv:1808.09657 [hep-lat]]
2018 arXiv
-
[28]
J. P. Lees et al. [BaBar Collaboration], Phys. Rev. Lett. 109 (2012) 101802 [arXiv:1205.5442 [hep-ex]]
2012 arXiv
-
[29]
J. P. Lees et al. [BaBar Collaboration], Phys. Rev. D 88 (2013) no.7, 072012 [arXiv:1303.0571 [hep-ex]]
2013 arXiv
-
[30]
Huschle et al
M. Huschle et al. [Belle Collaboration], Phys. Rev. D 92 (2015) no.7, 072014 [arXiv:1507.03233 [hep-ex]]
2015 arXiv
-
[31]
Hirose et al
S. Hirose et al. [Belle Collaboration], Phys. Rev. Lett. 118 (2017) no.21, 211801 [arXiv:1612.00529 [hep-ex]]
2017 arXiv
-
[32]
Hirose et al
S. Hirose et al. [Belle Collaboration], Phys. Rev. D 97 (2018) no.1, 012004 [arXiv:1709.00129 [hep-ex]]
2018 arXiv
-
[33]
Aaij et al
R. Aaij et al. [LHCb Collaboration], Phys. Rev. Lett. 115 (2015) no.11, 111803 Erratum: [Phys. Rev. Lett. 115 (2015) no.15, 159901] [arXiv:1506.08614 [hep-ex]]
2015
-
[34]
Aaij et al
R. Aaij et al. [LHCb Collaboration], Phys. Rev. Lett. 120 (2018) no.17, 171802 [arXiv:1708.08856 [hep-ex]]
2018 arXiv
-
[35]
Aaij et al
R. Aaij et al. [LHCb Collaboration], Phys. Rev. D 97 (2018) no.7, 072013 [arXiv:1711.02505 [hep-ex]]
2018 arXiv
-
[36]
Aaij et al
R. Aaij et al. [LHCb Collaboration], Phys. Rev. Lett. 120 (2018) no.12, 121801 [arXiv:1711.05623 [hep-ex]]
2018 arXiv
-
[37]
Abdesselam et al
A. Abdesselam et al. [Belle Collaboration], arXiv:1904.08794 [hep-ex]. 10 Constraints on New Physics from B mesons Monika Blanke
1904 arXiv
-
[38]
Blanke, A
M. Blanke, A. Crivellin, S. de Boer, T. Kitahara, M. Moscati, U. Nierste and I. NiÅ ˛ aandÅ¿iĢG, Phys. Rev. D 99 (2019) no.7, 075006 [arXiv:1811.09603 [hep-ph]]
2019 arXiv
-
[39]
Blanke, A
M. Blanke, A. Crivellin, T. Kitahara, M. Moscati, U. Nierste and I. Nišandži´c, arXiv:1905.08253 [hep-ph]
1905 arXiv
-
[40]
X. G. He and G. Valencia, Phys. Rev. D 87 (2013) no.1, 014014 [arXiv:1211.0348 [hep-ph]]
2013 arXiv
-
[41]
Greljo, G
A. Greljo, G. Isidori and D. Marzocca, JHEP 1507 (2015) 142 [arXiv:1506.01705 [hep-ph]]
2015 arXiv
-
[42]
D. A. Faroughy, A. Greljo and J. F. Kamenik, Phys. Lett. B 764 (2017) 126 [arXiv:1609.07138 [hep-ph]]
2017 arXiv
-
[43]
Kalinowski, Phys
J. Kalinowski, Phys. Lett. B 245 (1990) 201
1990
-
[44]
W. S. Hou, Phys. Rev. D 48 (1993) 2342
1993
-
[45]
Crivellin, C
A. Crivellin, C. Greub and A. Kokulu, Phys. Rev. D 86 (2012) 054014 [arXiv:1206.2634 [hep-ph]]
2012 arXiv
-
[46]
Freytsis, Z
M. Freytsis, Z. Ligeti and J. T. Ruderman, Phys. Rev. D 92 (2015) no.5, 054018 [arXiv:1506.08896 [hep-ph]]
2015 arXiv
- [47]
-
[48]
R. X. Shi, L. S. Geng, B. Grinstein, S. Jäger and J. Martin Camalich, arXiv:1905.08498 [hep-ph]
1905 arXiv
-
[49]
Aebischer, W
J. Aebischer, W. Altmannshofer, D. Guadagnoli, M. Reboud, P. Stangl and D. M. Straub, arXiv:1903.10434 [hep-ph]
1903 arXiv
-
[50]
N. G. Deshpande and A. Menon, JHEP 1301 (2013) 025 [arXiv:1208.4134 [hep-ph]]
2013 arXiv
-
[51]
Tanaka and R
M. Tanaka and R. Watanabe, Phys. Rev. D 87 (2013) no.3, 034028 [arXiv:1212.1878 [hep-ph]]
2013 arXiv
-
[52]
Sakaki, M
Y . Sakaki, M. Tanaka, A. Tayduganov and R. Watanabe, Phys. Rev. D88 (2013) no.9, 094012 [arXiv:1309.0301 [hep-ph]]
2013 arXiv
-
[53]
Alonso, B
R. Alonso, B. Grinstein and J. Martin Camalich, JHEP 1510 (2015) 184 [arXiv:1505.05164 [hep-ph]]
2015 arXiv
-
[54]
Calibbi, A
L. Calibbi, A. Crivellin and T. Ota, Phys. Rev. Lett. 115 (2015) 181801 [arXiv:1506.02661 [hep-ph]]
2015 arXiv
-
[55]
Fajfer and N
S. Fajfer and N. Kosnik, Phys. Lett. B 755 (2016) 270 [arXiv:1511.06024 [hep-ph]]
2016 arXiv
-
[56]
Bordone, C
M. Bordone, C. Cornella, J. Fuentes-Martin and G. Isidori, Phys. Lett. B 779 (2018) 317 [arXiv:1712.01368 [hep-ph]]
2018 arXiv
-
[57]
Greljo, J
A. Greljo, J. Martin Camalich and J. D. Ruiz-Alvarez, Phys. Rev. Lett. 122 (2019) no.13, 131803 [arXiv:1811.07920 [hep-ph]]
2019 arXiv
-
[58]
Becirevic, I
D. Becirevic, I. Dorsner, S. Fajfer, N. Kosnik, D. A. Faroughy and O. Sumensari, Phys. Rev. D 98 (2018) no.5, 055003 [arXiv:1806.05689 [hep-ph]]
2018 arXiv
- [59]
-
[60]
Alonso, B
R. Alonso, B. Grinstein and J. Martin Camalich, Phys. Rev. Lett. 118 (2017) no.8, 081802 [arXiv:1611.06676 [hep-ph]]
2017 arXiv
-
[61]
A. G. Akeroyd and C. H. Chen, Phys. Rev. D 96 (2017) no.7, 075011 [arXiv:1708.04072 [hep-ph]]
2017 arXiv
-
[62]
Nierste, S
U. Nierste, S. Trine and S. Westhoff, Phys. Rev. D 78 (2008) 015006 [arXiv:0801.4938 [hep-ph]]
2008 arXiv
-
[63]
Becirevic, S
D. Becirevic, S. Fajfer, I. Nisandzic and A. Tayduganov, arXiv:1602.03030 [hep-ph]
-
[64]
Celis, M
A. Celis, M. Jung, X. Q. Li and A. Pich, Phys. Lett. B 771 (2017) 168 [arXiv:1612.07757 [hep-ph]]. 11 Constraints on New Physics from B mesons Monika Blanke
2017 arXiv
-
[65]
Iguro, T
S. Iguro, T. Kitahara, Y . Omura, R. Watanabe and K. Yamamoto, JHEP1902 (2019) 194 [arXiv:1811.08899 [hep-ph]]
2019 arXiv
-
[66]
Becirevic, M
D. Becirevic, M. Fedele, I. Nisandzic and A. Tayduganov, arXiv:1907.02257 [hep-ph]
1907 arXiv
-
[67]
Crivellin, D
A. Crivellin, D. Mueller and T. Ota, JHEP 1709 (2017) 040 [arXiv:1703.09226 [hep-ph]]
2017 arXiv
-
[68]
Aloni, A
D. Aloni, A. Efrati, Y . Grossman and Y . Nir, JHEP1706 (2017) 019 [arXiv:1702.07356 [hep-ph]]
2017 arXiv
-
[69]
Aaij et al
R. Aaij et al. [LHCb Collaboration], JHEP 1602 (2016) 104 [arXiv:1512.04442 [hep-ex]]
2016 arXiv
-
[70]
Aaij et al
R. Aaij et al. [LHCb Collaboration], JHEP 1708 (2017) 055 [arXiv:1705.05802 [hep-ex]]
2017 arXiv
-
[71]
Aaij et al
R. Aaij et al. [LHCb Collaboration], Phys. Rev. Lett. 122 (2019) no.19, 191801 [arXiv:1903.09252 [hep-ex]]
2019 arXiv
-
[72]
Archilli and C
Contributions by F. Archilli and C. Marin, these proceedings
-
[73]
Alguero, B
M. Alguero, B. Capdevila, A. Crivellin, S. Descotes-Genon, P. Masjuan, J. Matias and J. Virto, arXiv:1903.09578 [hep-ph]
1903 arXiv
-
[74]
Arbey, T
A. Arbey, T. Hurth, F. Mahmoudi, D. M. Santos and S. Neshatpour, Phys. Rev. D 100 (2019) no.1, 015045 [arXiv:1904.08399 [hep-ph]]
2019 arXiv
- [75]
-
[76]
Aaboud et al
M. Aaboud et al. [ATLAS Collaboration], JHEP 1904 (2019) 098 [arXiv:1812.03017 [hep-ex]]
2019 arXiv
-
[77]
CMS Collaboration, CMS-PAS-BPH-16-004
-
[78]
Aaij et al
R. Aaij et al. [LHCb Collaboration], Phys. Rev. Lett. 118 (2017) no.19, 191801 [arXiv:1703.05747 [hep-ex]]
2017 arXiv
-
[79]
Alguero, B
M. Alguero, B. Capdevila, S. Descotes-Genon, P. Masjuan and J. Matias, Phys. Rev. D 99 (2019) no.7, 075017 [arXiv:1809.08447 [hep-ph]]
2019 arXiv
-
[80]
Crivellin, C
A. Crivellin, C. Greub, D. Mueller and F. Saturnino, Phys. Rev. Lett. 122 (2019) no.1, 011805 [arXiv:1807.02068 [hep-ph]]
2019 arXiv
-
[81]
Altmannshofer and D
W. Altmannshofer and D. M. Straub, Eur. Phys. J. C 73 (2013) 2646 [arXiv:1308.1501 [hep-ph]]
2013 arXiv
-
[82]
Gauld, F
R. Gauld, F. Goertz and U. Haisch, JHEP 1401 (2014) 069 [arXiv:1310.1082 [hep-ph]]
2014 arXiv
-
[83]
Altmannshofer, S
W. Altmannshofer, S. Gori, M. Pospelov and I. Yavin, Phys. Rev. D 89 (2014) 095033 [arXiv:1403.1269 [hep-ph]]
2014 arXiv
-
[84]
Crivellin, G
A. Crivellin, G. D’Ambrosio and J. Heeck, Phys. Rev. D 91 (2015) no.7, 075006 [arXiv:1503.03477 [hep-ph]]
2015 arXiv
-
[85]
Descotes-Genon, M
S. Descotes-Genon, M. Moscati and G. Ricciardi, Phys. Rev. D 98 (2018) no.11, 115030 [arXiv:1711.03101 [hep-ph]]
2018 arXiv
-
[86]
Gripaios, M
B. Gripaios, M. Nardecchia and S. A. Renner, JHEP 1606 (2016) 083 [arXiv:1509.05020 [hep-ph]]
2016 arXiv
-
[87]
Arnan, L
P. Arnan, L. Hofer, F. Mescia and A. Crivellin, JHEP 1704 (2017) 043 [arXiv:1608.07832 [hep-ph]]
2017 arXiv
-
[88]
Arnan, A
P. Arnan, A. Crivellin, M. Fedele and F. Mescia, JHEP 1906 (2019) 118 [arXiv:1904.05890 [hep-ph]]
2019 arXiv
-
[89]
Belanger, C
G. Belanger, C. Delaunay and S. Westhoff, Phys. Rev. D 92 (2015) 055021 [arXiv:1507.06660 [hep-ph]]
2015 arXiv
-
[90]
J. F. Kamenik, Y . Soreq and J. Zupan, Phys. Rev. D97 (2018) no.3, 035002 [arXiv:1704.06005 [hep-ph]]. 12 Constraints on New Physics from B mesons Monika Blanke
2018 arXiv
- [91]
-
[92]
Becirevic, S
D. Becirevic, S. Fajfer, N. Kosnik and O. Sumensari, Phys. Rev. D 94 (2016) no.11, 115021 [arXiv:1608.08501 [hep-ph]]
2016 arXiv
-
[93]
J. C. Pati and A. Salam, Phys. Rev. D 10 (1974) 275 doi:10.1103/PhysRevD.10.275, 10.1103/PhysRevD.11.703.2
1974 doi
-
[94]
P. Q. Hung, A. J. Buras and J. D. Bjorken, Phys. Rev. D 25 (1982) 805
1982
-
[95]
Valencia and S
G. Valencia and S. Willenbrock, Phys. Rev. D 50 (1994) 6843 [hep-ph/9409201]
1994 arXiv
-
[96]
Di Luzio, A
L. Di Luzio, A. Greljo and M. Nardecchia, Phys. Rev. D 96 (2017) no.11, 115011 [arXiv:1708.08450 [hep-ph]]
2017 arXiv
-
[97]
Calibbi, A
L. Calibbi, A. Crivellin and T. Li, Phys. Rev. D 98 (2018) no.11, 115002 [arXiv:1709.00692 [hep-ph]]
2018 arXiv
-
[98]
Greljo and B
A. Greljo and B. A. Stefanek, Phys. Lett. B 782 (2018) 131 [arXiv:1802.04274 [hep-ph]]
2018 arXiv
-
[99]
Balaji, R
S. Balaji, R. Foot and M. A. Schmidt, Phys. Rev. D 99 (2019) no.1, 015029 [arXiv:1809.07562 [hep-ph]]
2019 arXiv
-
[100]
Barbieri, C
R. Barbieri, C. W. Murphy and F. Senia, Eur. Phys. J. C 77 (2017) no.1, 8 [arXiv:1611.04930 [hep-ph]]
2017 arXiv
-
[101]
Blanke and A
M. Blanke and A. Crivellin, Phys. Rev. Lett. 121 (2018) no.1, 011801 [arXiv:1801.07256 [hep-ph]]
2018 arXiv
-
[102]
Cornella, J
C. Cornella, J. Fuentes-Martin and G. Isidori, JHEP 1907 (2019) 168 [arXiv:1903.11517 [hep-ph]]
2019 arXiv
-
[103]
Bona [UTfit Collaboration], PoS CKM 2016 (2017) 096
M. Bona [UTfit Collaboration], PoS CKM 2016 (2017) 096. Updates available on http://www.utfit.org/UTfit/
2017
-
[104]
Bai et al
Z. Bai et al. [RBC and UKQCD Collaborations], Phys. Rev. Lett. 115 (2015) no.21, 212001 [arXiv:1505.07863 [hep-lat]]
2015 arXiv
-
[105]
A. J. Buras and J. M. Gerard, JHEP 1512 (2015) 008 [arXiv:1507.06326 [hep-ph]]
2015 arXiv
-
[106]
A. J. Buras, M. Gorbahn, S. Jaeger and M. Jamin, JHEP 1511 (2015) 202 [arXiv:1507.06345 [hep-ph]]
2015 arXiv
-
[107]
Kitahara, U
T. Kitahara, U. Nierste and P. Tremper, JHEP 1612 (2016) 078 [arXiv:1607.06727 [hep-ph]]
2016 arXiv
-
[108]
A. J. Buras, arXiv:1812.06102 [hep-ph]
-
[109]
J. R. Batley et al. [NA48 Collaboration], Phys. Lett. B 544 (2002) 97 [hep-ex/0208009]
2002 arXiv
-
[110]
Alavi-Harati et al
A. Alavi-Harati et al. [KTeV Collaboration], Phys. Rev. D67 (2003) 012005 Erratum: [Phys. Rev. D 70 (2004) 079904] [hep-ex/0208007]
2003 arXiv
-
[111]
Abouzaid et al
E. Abouzaid et al. [KTeV Collaboration], Phys. Rev. D83 (2011) 092001 [arXiv:1011.0127 [hep-ex]]
2011 arXiv
-
[112]
A. J. Buras and J. M. Gerard, Eur. Phys. J. C 77 (2017) no.1, 10 [arXiv:1603.05686 [hep-ph]]
2017 arXiv
-
[113]
Gisbert and A
H. Gisbert and A. Pich, Rept. Prog. Phys. 81 (2018) no.7, 076201 [arXiv:1712.06147 [hep-ph]]
2018 arXiv
-
[114]
Blanke, A
M. Blanke, A. J. Buras and S. Recksiegel, Eur. Phys. J. C 76 (2016) no.4, 182 [arXiv:1507.06316 [hep-ph]]
2016 arXiv
-
[115]
A. J. Buras, D. Buttazzo and R. Knegjens, JHEP 1511 (2015) 166 [arXiv:1507.08672 [hep-ph]]. 13 Constraints on New Physics from B mesons Monika Blanke
2015 arXiv
-
[116]
A. J. Buras and F. De Fazio, JHEP 1603 (2016) 010 [arXiv:1512.02869 [hep-ph]]
2016 arXiv
-
[117]
Kitahara, U
T. Kitahara, U. Nierste and P. Tremper, Phys. Rev. Lett. 117 (2016) no.9, 091802 [arXiv:1604.07400 [hep-ph]]
2016 arXiv
-
[118]
Bobeth, A
C. Bobeth, A. J. Buras, A. Celis and M. Jung, JHEP 1704 (2017) 079 [arXiv:1609.04783 [hep-ph]]
2017 arXiv
-
[119]
M. Endo, T. Goto, T. Kitahara, S. Mishima, D. Ueda and K. Yamamoto, JHEP 1804 (2018) 019 [arXiv:1712.04959 [hep-ph]]
2018 arXiv
-
[120]
N. Haba, H. Umeeda and T. Yamada, JHEP 1805 (2018) 052 [arXiv:1802.09903 [hep-ph]]
2018 arXiv
-
[121]
A. J. Buras, D. Buttazzo, J. Girrbach-Noe and R. Knegjens, JHEP 1411 (2014) 121 [arXiv:1408.0728 [hep-ph]]
2014 arXiv
-
[122]
Cortina Gil et al
E. Cortina Gil et al. [NA62 Collaboration], Phys. Lett. B 791 (2019) 156 [arXiv:1811.08508 [hep-ex]]
2019 arXiv
-
[123]
J. K. Ahn et al. [KOTO Collaboration], Phys. Rev. Lett.122 (2019) no.2, 021802 [arXiv:1810.09655 [hep-ex]]
2019 arXiv
-
[124]
Ambrosino et al
F. Ambrosino et al. [KLEVER Project Collaboration], arXiv:1901.03099 [hep-ex]. 14
1901 arXiv
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