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This study aims to discriminate between Type I and Heterotic superstring models by observing cosmic magnetic fields and primordial gravitational waves. Theoretical constraints and experimental confrontations are performed to determine the allowed parameter space.
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Università degli Studi di Bari Facoltà di Scienze Matematiche, Fisiche e Naturali Dipartimento di Fisica & INFN Observable (?) cosmological signatures of superstrings in pre-big bang models of inflation Stefano Nicotri Based on PLB 633 155 (2006), with M. Gasperini
Main aim Discriminate between the Type I end the Heterotic superstring model through cross correlated observations of cosmic magnetic fields and primordial gravitational-waves background • Spectral energy density for photons (two models) • Spectral energy density for gravitons • Theoretical and phenomenological constraints • Plot of the allowed regions in the parameter space • Confrontation of the two models by experiments
Cosmic magnetic fields • Magnetic fields on galactic and intergalactic scales: • Amplitude ~ 10-6 Gauss • Coherence scale > 10 Kpc Possible mechanism of production Galactic Dynamo (Parker et al., 1973) It needs some “seed” magnetic field to be started up, that is a field which is strong enough to be amplificated by this mechanism.
Seeds Even in vacuum F 0 (quantum fluctuations) Inflationary expansion can amplificate quantum fluctuations Identification of the amplified quantum fluctuations with the seeds fields required by the dynamo to be started up.
Problem Conformal invariance of Maxwell lagrangian + Conformally flat metric Minimal coupling + = Fluctuations not coupled to geometry Inflation doesn’t amplificate the fluctuations
Possible solution Superstring theory predicts the existence of the dilaton , a scalar field which is non-minimally coupled to the E.M. field: e-F F depends on superstring model We compare the cases =1 (Heterotic superstring) and =1/2 (Type I superstring)
Action Internal space isotropy Ten dimensional space-time Action for the fluctuation fields i Equation of motion “pump field” which amplificates the fluctuations in the inflationary phase. It depends on the dilaton coupling and on the choice of the model of cosmological evolution, through the scale factors
Minimal pre-Big Bang Model s = 1/s 1 = 1/1
This choice determinates: • Pump field • Equation of motion (Bessel equation) • Solutions (amplification) We can get the physical parameters: Number of pairs produced from the vacuum Differential energy density Spectral energy density
Spectral energy density Photons Gravitons Free (?) parameters that we shall discuss later Photons spectrum is model dependent while gravitons spectrum is model independent
Constraints Constraints shared by both spectra: • Homogeneity • Nucleosyntesis • Growing spectrum Constraints for the E.M. spectrum Constraints for the gravitons spectrum • Visibility by AdvancedLIGO • Pulsar timing measurement • Seed condition
Free parameters • 1 : frequency inverse of the transition time from pre-bb to post-bb phase • s : frequency inverse of the transition time from dilaton to string phase • : phenomenological parameter that possibly takes into account the effects of the higher order corrections to the effective action • 0 : exponent of the external scale factor • : exponent of the internal scale factor • : quantity that parametrizes the coupling of the dilaton with the E.M field in the two superstring models we have considered • H1 : value of the Hubble parameter at 1 Ansatz: H1=Ms=0.1Mp 1 = (Ms/Mp)1/2 ·1011Hz and s are the only two continuous parameter 0, and can assume only discrete values 2-dimensional parameter space
Contribution from internal dimensions Internal dimensions do not give any substantial contribution How does superposition region change?
Remarks • Superposition between Type I photons and gravitons allowed regions • No superposition between Heterotic photons and gravitons allowed regions • These considerations are substanially not influenced by internal dimensions contributions
Physical interpretation Presence of a superposition region between gravitons and Type I photons Absence of a superposition region between gravitons and Heterotic photons An efficient production of magnetic “seeds” is compatible with the production of relic gravitons detectable by Advanced LIGO An efficient production of magnetic “seeds” is not compatible with the production of relic gravitons detectable by Advanced LIGO
Conclusions Direct experimental information on the primordial intensity of the photon-dilaton coupling and on the superstring model that best describes primordial cosmological evolution can be obtained
Experiments Experimental confirmation of the production of primordial magnetic seeds as predicted by pre-Big Bang models + Detection of relic gravitons by Advanced LIGO No detection of relic gravitons by Advanced LIGO = = Experimental support to Type I superstring model Experimental support to Heterotic superstring model
Thanks to R. Anglani, P. Colangelo, F. De Fazio, R. Ferrandes, M. Gasperini, M. Lucente, M. Ruggieri Thank you for patience and attention
Heterotic Photons = 1
Type I Photons = 1/2
Gravitons (model) independent
Solutions Equations of motion Cosmological expansion has NO effect on the fluctuations
Pump field Equation of motion in momentum space Solutions
Action Contribution coming from the dimensional reduction
Action for the fluctuations ? Z() is the “pump field” which apmlificates the fluctuations Evolution equation
Potential Bessel Equation
Equation of motion Potential
Homogeneity The energy density of the particles must be small enough to allow linearized treatment of the fluctuations All times and frequencies
Nucleosyntesis This constraint is slightly stronger than the previous. It prohibits too intense fields at the epoch of light nuclei formation
Seed condition Lower buond on energy density. It’s the minimal intensity that allows the dynamo to be started up. Well defined time and frequency
Growing spectrum Nucleosyntesis constraint does not allow the spectrum to be decreasing with frequency Model dependent
Advanced LIGO We are interested in the study of relic gravitational waves detectable from next generation interferometers Sensibility of Advanced LIGO ’s antennaefixes a lower bound on the energy density of the gravitons produced
Pulsars timing measurements Up to now no variation of the pulsar period has been found that can be explained by the presence of relic gravitational waves Energy density must be small enough for frequencies of the order of the inverse of observation time
Growing spectrum Gravitational stability = + Necessity of a growing spectrum Z() can’t grow too fast in the stringy phase Growing dilaton condition