Axion-Like Particles from Strings. Andreas Ringwald (DESY)

Similar documents
Physics Case for Axion or ALP DM. Andreas Ringwald (DESY)

Physics case for axions and other WISPs. Andreas Ringwald (DESY)

Science Case for / Physics Goals of ALPS-II. Andreas Ringwald for the ALPS Collaboration

Axions and Axion-Like Particles in the Dark Universe. Andreas Ringwald (DESY)

Phenomenological Aspects of Local String Models

Heterotic Brane World

Grand Unification and Strings:

Phenomenological Aspects of LARGE Volume Models

Theory and phenomenology of hidden U(1)s from string compactifications

String Compactifications and low-energy SUSY: The last attempts?

Strings, Exceptional Groups and Grand Unification

The discrete beauty of local GUTs

Light hidden U(1)s in LARGE volume string compactifications

SM*A*S*H. Standard Model * Axion * See-saw * Hidden PQ scalar inflation. Andreas Ringwald (DESY)

Crosschecks for Unification

The QCD Axion. Giovanni Villadoro

E 6 Spectra at the TeV Scale

Strings and Particle Physics

Hierarchy Problems in String Theory: An Overview of the Large Volume Scenario

Predictions from F-theory GUTs. (High vs. low-scale SUSY; proton decay)

Neutrinos and Fundamental Symmetries: L, CP, and CP T

Yang-Hwan Ahn Based on arxiv:

Geography on Heterotic Orbifolds

Hidden Sector Baryogenesis. Jason Kumar (Texas A&M University) w/ Bhaskar Dutta (hep-th/ ) and w/ B.D and Louis Leblond (hepth/ )

Topology in QCD and Axion Dark Matter. Andreas Ringwald (DESY)

(Mainly centered on theory developments)

Inverse See-saw in Supersymmetry

The Standard Model and beyond

Light Paraphotons and Minicharged Particles in Realistic Extensions of the Standard Model

Lecture 03. The Standard Model of Particle Physics. Part II The Higgs Boson Properties of the SM

Introduction to Supersymmetry

QCD axions with high scale inflation

Search for New Physics at the Milliscale

Heterotic Supersymmetry

Exceptional Supersymmetry. at the Large Hadron Collider

2T-physics and the Standard Model of Particles and Forces Itzhak Bars (USC)

Axions. Kerstin Helfrich. Seminar on Theoretical Particle Physics, / 31

Gauge Threshold Corrections for Local String Models

Dynamics of the Peccei-Quinn Scale

Non-Abelian SU(2) H and Two-Higgs Doublets

Kähler Potentials for Chiral Matter in Calabi-Yau String Compactifications

Axino Phenomenology in the Kim-Nilles mechanism

String Phenomenology

Little Higgs Models Theory & Phenomenology

The Standard Model of particle physics and beyond

Axion Cold Dark Matter with High Scale Inflation. Eung Jin Chun

Kähler Potentials for Chiral Matter in Calabi-Yau String Compactifications

Sterile Neutrinos from the Top Down

EDMs from the QCD θ term

arxiv:hep-ph/ v1 6 Feb 2004

Soft Supersymmetry Breaking Terms in String Compactifications

Supersymmetry Breaking

How does neutrino confine GUT and Cosmology? July T. Fukuyama Center of Quantum Universe, Okayama-U

F-theory and Particle Physics

A Derivation of the Standard Model. ``String Phenomenology 2015, Madrid, June 12, 2015 Based on Nucl.Phys. B883 (2014) with B.

Beyond the Standard Model

Kaluza-Klein Dark Matter

Ultra-Light Particles Beyond the Standard Model

Anomalies and Remnant Symmetries in Heterotic Constructions. Christoph Lüdeling

arxiv: v1 [hep-th] 6 Mar 2014

Fuzzy extra dimensions and particle physics models

Supersymmetry, Dark Matter, and Neutrinos

arxiv: v1 [hep-th] 22 Oct 2017

May 7, Physics Beyond the Standard Model. Francesco Fucito. Introduction. Standard. Model- Boson Sector. Standard. Model- Fermion Sector

November 24, Scalar Dark Matter from Grand Unified Theories. T. Daniel Brennan. Standard Model. Dark Matter. GUTs. Babu- Mohapatra Model

The Constrained E 6 SSM

Direct generation of a Majorana mass for the Neutron from exotic instantons!

Axions and other (Super-)WISPs

kev sterile Neutrino Dark Matter in Extensions of the Standard Model

Axion and axion-like particle searches in LUX and LZ. Maria Francesca Marzioni

Shedding Light on the Hidden Sector

Anomaly and gaugino mediation

Unification without Doublet-Triplet Splitting SUSY Exotics at the LHC

New Physics from Vector-Like Technicolor: Roman Pasechnik Lund University, THEP group

Axions Theory SLAC Summer Institute 2007

A short review of axion and axino parameters

Unified Dark Matter. SUSY2014 Stephen J. Lonsdale. The University of Melbourne. In collaboration with R.R. Volkas. arxiv:

Theory III: String Theory. presented by Dieter Lüst, MPI and LMU-München

Unification without Doublet-Triplet Splitting SUSY Exotics at the LHC

U(1) Gauge Extensions of the Standard Model

Split Supersymmetry A Model Building Approach

New Physics below the Fermi Scale. Mikhail Shaposhnikov

Patrick Kirchgaeßer 07. Januar 2016

A derivation of the Standard Model. Based on Nucl.Phys. B883 (2014) with B. Gato Rivera

Searching for axions and ALPs from string theory

Gauge-Higgs Unification on Flat Space Revised

Neutrino Models with Flavor Symmetry

+ µ 2 ) H (m 2 H 2

Solar Axions Globular Cluster Supernova 1987A Dark Matter Long-Range Force. Axion Landscape. Georg G. Raffelt, Max-Planck-Institut für Physik, München

SUSY and Exotics. UK HEP Forum"From the Tevatron to the LHC, Cosener s House, May /05/2009 Steve King, UK HEP Forum '09, Abingdon 1

New experiment for axion dark matter

Alternatives to the GUT Seesaw

Naturalizing SUSY with the relaxion and the inflaton

December 10, :42 World Scientific Review Volume - 9in x 6in zpr 09. Chapter 1

Lecture 03. The Standard Model of Particle Physics. Part III Extensions of the Standard Model

PHYSICS BEYOND SM AND LHC. (Corfu 2010)

Attacking Dark Forces with Intense Electron Beams at DESY

Axion and Dark Matter Studies in IBS

Physics Beyond the Standard Model at the LHC

The mass of the Higgs boson

Transcription:

Axion-Like Particles from Strings. Andreas Ringwald (DESY) Origin of Mass 2014, Odense, Denmark, May 19-22, 2014

Hints for intermediate scale axion-like particles > Number of astro and cosmo hints pointing to existence of intermediate scale axion-like particles (ALPs; ultra-light pseudo-scalars (pseudo Nambu-Goldstone bosons) coupling to photons) [talk by Joerg Jaeckel] Anomalous gamma transparency [Aharonian et al. 07; De Angelis et al 07; Aliu et al. 08; Simet et al 08; Sanchez-Conde et al. 09;... Horns,Meyer 12; Meyer et al. 13] [Meyer] Andreas Ringwald Axion-like Particles from Strings Origin of Mass 2014 Odense 19-22 May 2014 Page 2

Hints for intermediate scale axion-like particles > Number of astro and cosmo hints pointing to existence of intermediate scale axion-like particles (ALPs; ultra-light pseudo-scalars (pseudo Nambu-Goldstone bosons) coupling to photons) Anomalous gamma transparency Dark radiation and soft X-ray excess from clusters [Cicoli,Conlon,Quevedo 12; Higaki,Takahashi 12; Marsh,Conlon 13; Angus et al. 13] g a & p 0.5/4N e 1.4 10 13 GeV 1 [Boyer et al., Soft excess in Coma as observed by EUVE `04] for m a. 10 12 ev Andreas Ringwald Axion-like Particles from Strings Origin of Mass 2014 Odense 19-22 May 2014 Page 3

Hints for intermediate scale axion-like particles > Number of astro and cosmo hints pointing to existence of intermediate scale axion-like particles (ALPs; ultra-light pseudo-scalars (pseudo Nambu-Goldstone bosons) coupling to photons) [Boyarski et al.1402.4119] Anomalous gamma transparency Dark radiation and soft X-ray excess from clusters 3.55 kev line from clusters [Bulbul et al. 1402.2301, Boyarski et al.1402.4119; Higaki et al. 1402.6965; Jaeckel et al. 1402.7335] Andreas Ringwald Axion-like Particles from Strings Origin of Mass 2014 Odense 19-22 May 2014 Page 4

Hints for intermediate scale axion-like particles > Number of astro and cosmo hints pointing to existence of intermediate scale axion-like particles (ALPs; ultra-light pseudo-scalars (pseudo Nambu-Goldstone bosons) coupling to photons) Anomalous gamma transparency Dark radiation and soft X-ray excess from clusters 3.55 kev line from clusters > Require (2-3) ALPs in addition to axion Log 10»g ag» @GeV -1 D - 8-10 - 12-14 - 16-18 SN1987A g - Ray Burst Quasar Polarization PIXIEê PRISM Massive Stars Soft X - Ray Excess from Com a ALP CDM g - Ray Transparency Axion ALPS -II Haloscopes IAXO Axion CDM - 20-40 - 38-36 - 34-32 - 30-28 - 26-24 - 22-20 - 18-16 - 14-12 - 10-8 - 6-4 - 2 0 2 4 Log 10 m a @evd [Dias,Machado,Nishi,AR,Vaudrevange 1403.5760] 3.55 kev Line from Decaying ALP DM Andreas Ringwald Axion-like Particles from Strings Origin of Mass 2014 Odense 19-22 May 2014 Page 5

UV completions yielding intermediate scale axion/alps > Ad-hoc UV completions: [Peccei,Quinn `77; Kim `79; Shifman et al. `80; Dine et al. `81;...] Add one/more hidden complex scalar fields to the SM, whose vevs anomalous chiral Peccei-Quinn symmetries, U(1) PQi i(x) = 1 p 2 vi + i (x) e ia0 i (x)/f a 0 i At energies much below the symmetry breaking scales is that of Nambu-Goldstone bosons, v i v i break global, the low-energy effective field with decay constants f a 0 i = v i, which can be chosen ad hoc at intermediate scales. The axionic couplings C ij arise due fermionic SM-SM- U(1) PQi chiral triangle anomalies and depend on the particular PQ charge assignments of the fermions in the model, e.g. KSVZ: all SM fermions have no PQ charge; one vector-like extra color triplet with chiral PQ assignment: DFSZ: two Higgs doublets H u,h d ; SM fermions have PQ charge; no extra fermion: Andreas Ringwald Axion-like Particles from Strings Origin of Mass 2014 Odense 19-22 May 2014 Page 6

UV completions yielding intermediate scale axion/alps The proper QCD axion solving the strong CP problem is the linear combination The ALPs are living in the space perpendicular to the axion. They are still Nambu- Goldstone bosons and do not couple to gluons. E.g. in case with two axion-like fields, A f A = C 1g a 0 1 f a 0 1 + C 2g a 0 2 f a 0 2, a f a = C 2g a 0 1 f a 0 2 + C 1g a 0 2 f a 0 1, with normalization 1 f 2 A = 1 f 2 a = C1g f a 0 1 2 + 2 C2g f a 0 2 Andreas Ringwald Axion-like Particles from Strings Origin of Mass 2014 Odense 19-22 May 2014 Page 7

UV completions yielding intermediate scale axion/alps > Drawbacks of these ad hoc models: 1. Hidden complex scalars introduced by hand 2. PQ symmetries introduced by hand 3. PQ symmetry breaking scales introduced by hand 4. Axion/ALPs not protected from explicit symmetry breaking effects due to higher dimensional operators modifying their potential, potentially shifting their minima away from zero Can be disastrous for the axionic solution of the strong CP problem: need to require Can make axion/alps too massive, > Concentrate on ALPs from strings which automatically avoid most of these drawbacks Closed string axion and ALPs in IIB string theory Accidental axion and ALPs in heterotic orbifolds Andreas Ringwald Axion-like Particles from Strings Origin of Mass 2014 Odense 19-22 May 2014 Page 8

Closed string ALPs in string theory 1. Massless bosonic spectrum of closed string sector of string theories in 10D contains form fields satisfying gauge symmetries 2. Symmetries broken by compactification [Quevedo `02] 3. Kaluza-Klein decomposition contains ALPs, with decay constants determined by string or compactification scale [Witten 84; Conlon 06; Svrcek,Witten 06] 4. Shift symmetries only violated through non-perturbative effects Andreas Ringwald Axion-like Particles from Strings Origin of Mass 2014 Odense 19-22 May 2014 Page 9

Closed string ALPs in IIB string theory > Concentrate on IIB case: Realisation of brane-world scenarios Visible sector gauge theory realized by stacks of D7 branes wrapping small 4-cycles Gravity propagates in the bulk, leading to a string scale and a KK scale possibly much much smaller than the Planck scale, at the expense of a large compactification volume [Jaeckel,AR `10] Andreas Ringwald Axion-like Particles from Strings Origin of Mass 2014 Odense 19-22 May 2014 Page 10

Closed string ALPs in IIB string theory > KK reduction (expansion in harmonic forms): > Number of ALPs determined by topology of CY orientifold: number of topologically non-equivalent 2-cycles or 4-cycles [Kreuzer,Skarke] > An axiverse may naturally arise from strings [Arvanitaki et al. `09] Andreas Ringwald Axion-like Particles from Strings Origin of Mass 2014 Odense 19-22 May 2014 Page 11

Closed string ALPs in IIB string theory > Each axion-like field comes along with a real scalar field saxion-like field which is real part of lowest component of chiral superfield, Kähler modulus measuring the volume of 4-cycle > 4D EFT [Jockers, Louis `05] from KK reduction of D-brane action, volume measures gauge coupling, has axionic coupling, Andreas Ringwald Axion-like Particles from Strings Origin of Mass 2014 Odense 19-22 May 2014 Page 12

Closed string ALPs in LARGE volume IIB string theory > LVS requires at least four 4-cyles: [Cicoli et al. `11] bulk (large volume) cycle, size fixed perturbatively dp cycle, size fixed non-perturbatively cycle supporting the stack of branes describing the visible sector, size fixed perturbatively cycle supporting a stack of branes providing D-terms to stabilise the volume of the visible cycle > LVS has at least two light ALPs: [Cicoli, Goodsell, AR, 1206.0819] large volume ALP small coupling, a 0 b with C bvs ' O V 2/3 a 0 vs visible sector ALP with, ) or eaten by Abe- either heavy ( lian gauge field Andreas Ringwald Axion-like Particles from Strings Origin of Mass 2014 Odense 19-22 May 2014 Page 13

Closed string ALPs in LARGE volume IIB string theory > LVS requires at least four 4-cyles: [Cicoli et al. `11] bulk (large volume) cycle, size fixed perturbatively dp cycle, size fixed non-perturbatively cycle supporting the stack of branes describing the visible sector, size fixed perturbatively cycle supporting a stack of branes providing D-terms to stabilise the volume of the visible cycle > LVS has at least two light ALPs: [Cicoli, Goodsell, AR, 1206.0819] large volume ALP small coupling, a 0 b with C bvs ' O V 2/3 a 0 vs visible sector ALP with, either heavy ( ) or eaten by Abelian gauge field > More light ALPs if there are more small cycles intersecting visible sector branes Andreas Ringwald Axion-like Particles from Strings Origin of Mass 2014 Odense 19-22 May 2014 Page 14

Closed string ALPs in LARGE volume IIB string theory > Mass scales for : > 4D EFT of LVS with intermediate string scale may offer ALP explanation of astrophysical hints, since in this scenario naturally more than one ALP with Andreas Ringwald Axion-like Particles from Strings Origin of Mass 2014 Odense 19-22 May 2014 Page 15

Accidental ALPs in heterotic orbifold compactifications 1. Plenitude of hidden complex scalar fields in orbifold compactifications 2. Multitude of discrete symmetries which are exact at perturbative level R-symmetries from the broken SO(6) symmetry of compact space Stringy discrete symmetries from joining and splitting of strings 3. PQ symmetries can occur in the low-energy EFT as accidental remnants of these discrete symmetries, that is the discrete symmetries forbid explicit PQ symmetry violating operators up to a certain mass dimension in low-energy effective Lagrangian [Choi,Kim,Kim 07; Choi,Nilles,Ramos-Sanchez,Vaudrevange 09] 4. Axion/ALP mass protected if discrete symmetries large Andreas Ringwald Axion-like Particles from Strings Origin of Mass 2014 Odense 19-22 May 2014 Page 16

Accidental ALPs in heterotic orbifold compactifications > Ad-hoc example: (DFSZ x KVSZ)-like model featuring sym. Z 13 Z 5 Z 0 5 Only allowed Yukawa couplings: Neutrino see-saw relations No flavour-changing neutral currents, since there is only one Higgs doublet for each type of fermion At mass dimension four, model has four accidental global U(1)s: U(1) B, ensuring baryon number conservation of ordinary quarks U(1) Q, ensuring conservation of the number of the exotic color triplet U(1) PQi, two Peccei-Quinn symmetries, whose charge assignments can be chosen as Andreas Ringwald Axion-like Particles from Strings Origin of Mass 2014 Odense 19-22 May 2014 Page 17

Accidental ALPs in heterotic orbifold compactifications Lowest dimensional operators respecting discrete symmetry, but breaking PQ symmetries, have mass dimension 14 or higher, inducing masses Model has gauge coupling unification close to intermediate scale, M U 10 13 GeV Αi 1 M 45. 42.5 40. 37.5 35. 32.5 30. 27.5 1 Α 1 1 Α 2 1 Α 3 10 9 10 10 10 11 10 12 10 13 M GeV Can be embedded in non-minimal SU(5) GUT [Dias,Franco,Pleitez 07] Proton stabilized since SU(5) multiplets involve beyond SM exotics and due to discrete symmetry Andreas Ringwald Axion-like Particles from Strings Origin of Mass 2014 Odense 19-22 May 2014 Page 18

Accidental ALPs in heterotic orbifold compactifications > For intermediate scales, model has axion plus ALP in astro-hint range: Andreas Ringwald Axion-like Particles from Strings Origin of Mass 2014 Odense 19-22 May 2014 Page 19

Accidental ALPs in heterotic orbifold compactifications > Mini-landscape of 348 MSSM-like models in Z6-II orbifold compactifications [Nilles,Vaudrevange1403.1597] SM gauge group 3 generations of quarks and leptons 1 (or more) Higgs pairs Further exotics: vector-like under SM gauge group O(100) hidden (SM singlet) complex scalars > Ongoing search for accidental ALPs [AR,Vaudrevange in prep.] Created all terms in superpotential up to order 6 in fields respecting discrete sym.: from strings splitting and joining from broken SO(6) Lorentz symmetry of compact space [Nilles et al. 1308.3435; Cabo Bizet et al. 1308.5669] Andreas Ringwald Axion-like Particles from Strings Origin of Mass 2014 Odense 19-22 May 2014 Page 20

Accidental ALPs in heterotic orbifold compactifications Determined the accidental U(1) global symmetries: found models with many of them, up to O(100) Determine the SM-SM- U(1) global triangle anomalies to find the accidental PQ symmetries and the couplings of the ALPs to SM gauge bosons Break U(1) global at intermediate scales and analyze couplings Which terms in superpotential break U(1) global explicitly? ALP masses? Andreas Ringwald Axion-like Particles from Strings Origin of Mass 2014 Odense 19-22 May 2014 Page 21

Summary and conclusions > Models that exhibit a QCD axion with an intermediate-scale decay constant and additional even lighter axion-like particles having the same decay constant and coupling to the photon can explain astrophysical anomalies and be tested in the next generation of helioscopes and light-shining-through-walls experiments > String phenomenology holds the promise of an axiverse the QCD axion plus a (possibly large) number of further ultralight axion-like particles, possibly populating each decade of mass down to the inverse Hubble scale > Promise fulfilled in LARGE Volume Scenario of IIB string compactifications and orbifold compactifications of the heterotic string Andreas Ringwald Axion-like Particles from Strings Origin of Mass 2014 Odense 19-22 May 2014 Page 22