# Dark Forces at Accelerators

Europe/Rome
Aula B. Touschek, Bldg 36 (INFN-LNF)

### Aula B. Touschek, Bldg 36

#### INFN-LNF

Via E. Fermi, 40 00044 Frascati Italy
Description
Several recent astrophysical observations have revived the idea of the existence of a hidden force weakly coupled to ordinary matter, mediated by new gauge bosons of masses in the MeV to GeV range. These new bosons can be produced at present day accelerators, both in collider experiments and in fixed target ones. A first successful meeting to discuss these issues was held in September 2009 at SLAC. At the time, new experimental activities were announced to start in several different laboratories. This workshop intends to bring theorists and experimentalists together to make the point on the advances in the field since then. The connection of these studies to the search for dark matter, as well as the potentials of future facilities, presently under study, will also be addressed.
Participants
• Achim Denig
• Aldo Morselli
• Alessandro Gaz
• Andrzej Kupsc
• Antonio De Santis
• Attila Krasznahorkay
• Barbara Sciascia
• Carl-Oscar Gullstroem
• Caterina Bloise
• Celine Boehm
• Chris kouvaris
• Christopher Wallace
• Danilo Babusci
• Dario Moricciani
• Elisa Guido
• Enrico Graziani
• Fabio Bossi
• Francesca Curciarello
• Frank Maas
• Gianfranco Morello
• Giorgio Giardina
• Giuseppe Mandaglio
• Graziano Venanzoni
• Harald Merkel
• Igal Jaegle
• Ivano Sarra
• James Beacham
• James Boyce
• Jan Stark
• Jaroslaw Zdebik
• Jinlin Fu
• Joerg Jaeckel
• John Jaros
• Lorenzo Pagnanini
• Marco Battaglieri
• Marco Ricci
• Matteo Mascolo
• Maxim Pospelov
• Michal Silarski
• Natalia Toro
• Norraphat Srimanobhas
• Oliver Baker
• Paolo Fermani
• Paolo Santangelo
• Pawel Moskal
• Pierre Fayet
• Raffaella De Vita
• Riccardo Cerulli
• Riccardo Faccini
• Rouven Essig
• Sarah Andreas
• Sergiy Ivashyn
• Silvia Galli
• Simona Giovannella
• Tobias Beranek
• Veerle Heijne
• William Marciano
• Yousuke Kataoka
Support
• Tuesday, 16 October
• 08:30 09:30
Registration 1h Room T-75 ()

### Room T-75

Registration

• 09:30 09:45
Workshop opening 15m Aula B. Touschek, Bldg 36

### Aula B. Touschek, Bldg 36

#### INFN-LNF

Via E. Fermi, 40 00044 Frascati Italy
• 09:45 10:55
Fixed target experiments I Aula B. Touschek, Bldg 36

### Aula B. Touschek, Bldg 36

#### INFN-LNF

Via E. Fermi, 40 00044 Frascati Italy
• 09:45
Dark forces and New Physics at the Intensity Frontier 35m
I review theoretical motivations for the experimental searches of new very weakly coupled states, and argue why this will continue to be an important part of the precision and intensity frontier programs.
Speaker: Dr Maxim Pospelov (Perimeter Institute/University of Victoria)
• 10:20
APEX: A Prime EXperiment 35m
APEX is a fixed target experiment at Thomas Jefferson National Accelerator Facility (JLab) in Virginia, USA, that searches for a new gauge boson (A') with sub-GeV mass and coupling to ordinary matter of g' ~ (10^-2 - 10^-6) e. Electrons impinge upon a fixed target of high-Z material to produce an A' via a process analogous to photon bremsstrahlung, which then decays to an e+ e- pair that is detected by the JLab Hall A High Resolution Spectrometers. A test run was held in July of 2010, covering an A' mass range from 175 to 250 MeV and couplings g'/e > 10^-3 . A full run is approved and will cover m_A' ~ 65 to 525 MeV and g'/e > 2.3x10^-4 . I will present the results of the test run and report on the current status of preparations for the full run.
Speaker: James Beacham (New York University)
• 10:55 11:25
coffee break 30m Aula B. Touschek, Bldg 36

### Aula B. Touschek, Bldg 36

#### INFN-LNF

Via E. Fermi, 40 00044 Frascati Italy
• 11:25 13:10
Fixed target experiments II Aula B. Touschek, Bldg 36

### Aula B. Touschek, Bldg 36

#### INFN-LNF

Via E. Fermi, 40 00044 Frascati Italy
• 11:25
Search for Dark Photons at the Mainz Microtron 35m
As a high intensity and high beam quality electron accelerator, the Mainz Microtron (MAMI) is well suited for the search for possible gauge bosons of the dark sector, the so called dark photons. The capabilities of the accelerator in combination with the high resolution spectrometer setup of the A1 collaboration were already demonstrated in a first test experiment in 2011. An extension of this experiment to lower photon masses took place beginning of this year and will be presented in this talk.
Speaker: Dr Harald Merkel (Institut fuer Kernphysik, Johannes Gutenberg-Uniververitaet Mainz)
• 12:00
Light Dark Gauge Boson Searches in Electron-Proton Scattering: Description of Present Data and Simulation for Future Experiments 35m
We study the exploration reach of various fixed target experiments searching for the dark photon. Therefore we investigate the creation of a lepton pair induced by quasi elastic scattering of an electron beam off a heavy nucleus (A,Z), i.e. e(A,Z) -> e (A,Z) e^+e^- with a dark photon A' as signal and a virtual photon as background in the intermediate state. We present our calculations in comparison with the data taken in the 2011 test runs of the MAMI dark photon experiment at Mainz and the APEX experiment at Jefferson Lab and prove the extracted exclusion limits on the kinetic mixing factor, describing the coupling strength of A' to leptons. Predictions of the expected exclusion limits of the 2012 beam time at MAMI will be presented. Furthermore estimates for the reach of the HPS and DarkLight experiments at Jefferson Lab and for the planned MESA facility at Mainz will be given.
Speaker: Tobias Beranek (Johannes Gutenberg University Mainz)
• 12:35
Hidden Photons in beam dump experiments 35m
Recently there has been much interest in hidden sectors with light extra U(1) gauge bosons, so called hidden photons. On the theoretical side, scenarios of that kind are well motivated as a common feature of physics beyond the Standard Model like string theory and SUSY. Because of their possible connection with dark matter they received further attention also from a phenomenological point of view triggered by different astrophysical anomalies and dark matter direct detection claims. In this talk, limits on hidden photons from past electron beam dump experiments will be shown including two new limits from such experiments at KEK and Orsay that have so far not been considered. In addition, the features of an extension to a simple supersymmetric hidden sector model with a viable Dark Matter candidate are presented.
Speaker: Sarah Andreas (DESY)
• 13:10 14:50
Lunch break 1h 40m Enea canteen ()

### Enea canteen

• 14:50 16:00
Fixed target experiments III Aula B. Touschek, Bldg 36

### Aula B. Touschek, Bldg 36

#### INFN-LNF

Via E. Fermi, 40 00044 Frascati Italy
• 14:50
Heavy Photon Search Experiment 35m
The Heavy Photon Search Experiment (HPS) is a new experiment at Jefferson Lab designed to look for massive vector gauge bosons (heavy photons) in the mass range 20-1000 MeV that couple to electrons with couplings ’/ in the range 10-5 to 10-10 . The experiment utilizes a compact forward spectrometer employing silicon microstrip detectors for vertexing and tracking and a PbWO4 electromagnetic calorimeter for fast triggering, and is designed to measure the invariant mass and decay vertex location of electro-produced heavy photons. Following initial approval in January 2011, the HPS Collaboration has mounted the HPS Test Run Experiment, which ran parasitically in Hall B at JLAB during Spring 2012, and commissioned the tracker, ECal, high rate trigger, and DAQ, and succeeded in testing background assumptions for the full experiment. On the basis of this successful test run, the experiment has been approved for physics running. The design, performance, and results from the Test Run apparatus will be discussed, along with the collaboration’s plans for future construction and data taking.
Speaker: John Jaros (SLAC)
• 15:25
The DarkLight Experiment – A Status Report 35m
Interest in experiments probing physics Beyond the Standard Model (BSM) has increased in recent years. At Jefferson Lab, the LIPSS experiments demonstrated that new, high intensity accelerators can be used to explore regions of dark matter parameter space heretofore inaccessible. The status of promising experiments will be discussed, with a focus on DarkLight, one of three efforts at Jefferson Lab searching for the gauge boson A’. DarkLight will use a high current electron beam scattering off a gaseous hydrogen target.
Speaker: Jim Boyce (Jlab)
• 16:00 16:30
coffee break 30m Aula B. Touschek, Bldg 36

### Aula B. Touschek, Bldg 36

#### INFN-LNF

Via E. Fermi, 40 00044 Frascati Italy
• 16:30 18:30
Meson and nuclear decays Aula B. Touschek, Bldg 36

### Aula B. Touschek, Bldg 36

#### INFN-LNF

Via E. Fermi, 40 00044 Frascati Italy
• 16:30
U boson search in phi dalitz decays with KLOE 35m
We have searched for a new neutral gauge vector boson (U boson) in phi(1020) to eta e+e- decays, using about 1.8 fb-1 of data collected by the KLOE detector. The present analysis is based on an identication of the eta meson by its decays into three neutral pions, which provides a sample about twice larger than the one used in our previously published result. The limit on U boson production is improved accordingly.
Speaker: Ivano Sarra (LNF)
• 17:05
Search for a new gauge boson in π0 decays with WASA-at-COSY 35m
Decays of the π0 allows to search mediates gauge bosons of dark forces in the MeV range. The decay π 0 → e+ e−γ is sensitive to a "dark photon" that decays into an e+ e− pair. WASA-at-COSY has collected a 500k data sample to constrains the parameters of this hypothetical gauge boson. The rare decay π 0 → e+ e− might also probe physics beyond the standard model. The 3σ deviation between experiment and SM prediction might be explained by a dark gauge boson, which might also account for the enhanced e+ e− annihilation line from the galactic center. A high statistics run with WASA-at-COSY could confirm the present experimental result.
Speaker: Mr Carl-Oscar Gullstroem (Uppsala University)
• 17:40
Search for a light neutral boson in nuclear transitions 35m
In a recent series of papers the intriguing possibility was explored that the cosmic dark matter consists of new elementary particles with masses in the MeV range, which could be searched for in nuclear physics laboratories. Such particles are not excluded by any obvious laboratory measurements or astrophysical arguments. There are even some experimental indications for a light neutral boson with a mass of around 9 MeV/c2 [1,2]. The spectrometers used for the above studies were plastic telescopes, which are insufficient for the required precision. We have improved the setups already and got somewhat stronger indications, but the reliability of the results can still be questioned because of the large systematic errors [3,4]. The signature of the new particle is the very characteristic angular correlation of the e+e- pairs from their decay. Quantum electrodynamics predicts that the angular correlation between the e+e- pairs emitted in internal pair creation drops smoothly with the separation angle. In striking contrast, when the transition takes place by the emission of a short-lived neutral particle annihilating into an e$^+$e$^-$ pair, the angular correlation becomes sharply peaked at large angles. In order to search for this signature with high confidence we need an internal pair spectrometer with much better specifications, which was ever built for studying nuclear transitions. We started to build a Compact Orange type Positron Electron spectrometer (COPE) for precise studies of the e+e- pair creation in the energy range of 10-20 MeV with large solid angle, good energy (1\%) and angular (2 deg.) resolutions, using strong permanent magnets. The diameter of such a spectrometer will be about 30 cm, which is versatile and can be used at different laboratories. With the presently available tracking detectors, data-acquisition systems and computers we will be able to study the differential internal pair creation process more precisely than ever before, with a precision enaugh for confirming (or discarding with high confidence) the existence of such light neutral particles. References: [1] F.W.N. de Boer and R. van Dantzig, Phys. Rev. Lett. 61, 1274 (1988). [2] F.W.N. de Boer et al., Phy. Lett. B 388, 235. (1996); J. Phys. G 23, L85 (1997); J. Phys. G 27 L29 (2001). [3] A. Krasznahorkay et al., Acta Phys. Polonica B 37, 239 (2006); Nucl. Phys. News Int. 15, 36 (2005); AIP Conf. Proc. 802, 236 (2005). [4] A. Vitez et al., Acta Phys. Polonica B 39 (2008) 483.
Speaker: Prof. Attila Krasznahorkay (Inst. of Nucl. Res. of the Hung. Acad. of Sci. (ATOMKI), Head, Division of Nuclear Physics)
• 18:30 20:00
Welcome Cocktail 1h 30m Aula B. Touschek, Bldg 36

### Aula B. Touschek, Bldg 36

#### INFN-LNF

Via E. Fermi, 40 00044 Frascati Italy
• Wednesday, 17 October
• 08:45 11:05
Electron-positron collider experiments I Aula B. Touschek, Bldg 36

### Aula B. Touschek, Bldg 36

#### INFN-LNF

Via E. Fermi, 40 00044 Frascati Italy
• 08:45
U bosons, "dark" or "hidden" photons, extra U(1)'s and new forces 35m
Speaker: Prof. Pierre Fayet (ENS Paris)
• 09:20
Searches for dark photons at BABAR 35m
We present the results of several searches for dark photons produced in e+e- collisions and decaying into leptons, hadrons, or invisible final states.
Speaker: Elisa Guido (INFN Genova)
• 09:55
U-Boson search in $e^+e^- \to \mu^+\mu^-(\gamma)$ process at KLOE 35m
Following recent puzzling astrophysical results and recent theoretical studies, a search for a relatively low mass ( 1 GeV) new vector boson (the U), weakly coupled with SM particles and decaying into leptons pairs, by using the Initial State Radiation (ISR) process, was performed at KLOE. The KLOE experiment at the $\phi$ − factory DA$\Phi$NE is the first to have exploited ISR to precisely determine cross section process like $e^+e^- \to \pi^+\pi^-(\gamma)$ and $e^+e^- \to \mu^+\mu^-(\gamma)$ cross section below 1 GeV. We use 220 pb$^-1$ of data to search for light vector boson in the $e^+e^- \to \mu^+\mu^-(\gamma)$ channel. No evidence was found and a prelimiary upper limit in the mass range 600 - 1000 MeV was extracted.
Speaker: Dr Francesca Curciarello (Dipartimento di Fisica-Università di Messina)
• 10:30
Search for dark sector at BESIII 35m
At BESIII, with 106 million psi(2S) events at BESIII, we have searched for a light Higgs-like boson A0 in the process psi(2S)-> pi+pi- J/psi, J/psi->\gamma A0, A0-> mu+mu-. We set 90% confidence level upper limits on the product branching fractions for J/psi -> gammaA0, A0 -> mu+mu− that range from 4 * 10^−7 to 2.1 * 10^−5, depending on the mass of A0, for M(A0) < 3.0 GeV/c2. Using J/psi-> \phi eta, phi \etap in 225 million J/psi decay events, we also make an updated analysis for \eta /\etap -> invisible decay. No evidence is found for these rare decays, and upper limits at 90\% confidence level are set, which are 5-10 times stringent than previous limits set by the previous BESII experiment.
Speaker: Mr Jinlin Fu (Nanjing University)
• 11:05 11:35
coffee break 30m Aula B. Touschek, Bldg 36

### Aula B. Touschek, Bldg 36

#### INFN-LNF

Via E. Fermi, 40 00044 Frascati Italy
• 11:35 13:20
Electron-positron collider experiments II Aula B. Touschek, Bldg 36

### Aula B. Touschek, Bldg 36

#### INFN-LNF

Via E. Fermi, 40 00044 Frascati Italy
• 11:35
Dark photon search and the Higgs-strahlung channel 35m
Many extensions of the Standard Model introduce an additional U(1) interaction, which is mediated by a U(1) boson, often by a Higgs mechanism adding a dark Higgs (or dark Higgses) to the models. This gauge boson, also known as the "Dark Photon", typically has very weak coupling to Standard Model particles. Experimental results from direct Dark Matter searches, (e.g. DAMA/LIBRA) and other experimental anomalies (e.g. g-2), can be explained by such an additional interaction. Dark gauge bosons are typically of low mass; of order MeV to GeV. The ideal tools to discover such particles are therefore not high-energy collider experiments, but lower-energy high-luminosity collider experiments like Belle and BaBar, or dedicated fixed target experiments, several of which are planned or already under construction at JLAB (Newport News, USA) or at MAMI (Mainz, Germany), for example. In Belle, the search of the dark photon focuses on the so-called Higgs-strahlung channel, as proposed by Batell et al., where a dark photon and a dark Higgs are produced. Preliminary results will be presented and discussed. B. Batell, M. Pospelov, and A. Ritz arXiv:0903.0363 (2009).
Speaker: Dr Igal Jaegle (University of Hawaii)
• 12:10
Search for dark photon and dark Higgs at BABAR 35m
We have searched for a dark photon produced in e+e- collisions and radiating a dark Higgs. The resulting 6-fermion final state is reconstructed in leptonic and leptonic+hadronic channels. We find no signal and set tight limits on the parameters of the model.
Speaker: Alessandro Gaz (University of Colorado)
• 12:45
Search for dark higgsstrahlung processes at KLOE 35m
We searched for the existence of a higgsstrahlung process in a secluded sector, possibly leading to a dark photon and a dark Higgs boson final state. Using the KLOE detector at DAFNE, we investigated the case in which the dark Higgs boson is lighter than the dark photon U and thus escapes detection, showing up as missing energy, and the dark photon U decays in a muon pair. We will report the status of the analysis.
Speaker: Enrico Graziani (ROMA3)
• 13:20 14:50
lunch break 1h 30m Enea canteen ()

### Enea canteen

• 14:50 16:00
Hadron collider experiments Aula B. Touschek, Bldg 36

### Aula B. Touschek, Bldg 36

#### INFN-LNF

Via E. Fermi, 40 00044 Frascati Italy
• 14:50
Search for long lived exotic particles at LHCb 35m
Several theories beyond the Standard Model predict the existence of new long-lived particles. We present results from searches of LHCb data for secondary vertices which can be associated with the decay of such particles, and set limits on the associated production rates.
Speaker: Veerle Heijne (NIKHEF)
• 15:25
Search for invisible particle production in monojet and monophoton events with missing transverse momentum with the ATLAS detector 35m
Events composed of one high transverse energy jet or photon and large missing transverse momentum represent one of the simplest and most striking signatures that can be observed at a hadron collider. The Standard Model contribution to 'monojet' events is dominated by a Z decaying to a pair of neutrinos plus a recoiling jet. Several new physics models predict monojet and monophoton events. They can occur via production of a jet/photon in association with an invisible particle or via pair production of invisible particles recoiling against a hard radiative jet or photon. The talk presents results from searches for new physics in monojet and monophoton events performed by the ATLAS experiment at the LHC.
Speaker: Jan Stark (LPSC Grenoble)
• 16:00 16:30
coffee break 30m Aula B. Touschek, Bldg 36

### Aula B. Touschek, Bldg 36

#### INFN-LNF

Via E. Fermi, 40 00044 Frascati Italy
• Thursday, 18 October
• 08:45 11:05
Particdle dark matter I Aula B. Touschek, Bldg 36

### Aula B. Touschek, Bldg 36

#### INFN-LNF

Via E. Fermi, 40 00044 Frascati Italy
• 08:45
Dark Matter candidates: where do we stand? 35m
I will review the different dark matter candidates which have been proposed during the last few years, recalling in particular the motivation for introducing them and will discuss the type of dark forces which have been proposed in these new models.
Speaker: Celine Boehm (Durahm)
• 09:20
Direct detection of Dark Matter particles 35m
In the direct investigation of the Dark Matter particles in the galactic halo both model independent and model dependent strategies with various target materials are exploited. In particular, recent results obtained by the DAMA/LIBRA set-up, exploiting the model independent annual modulation signature for Dark Matter particles, will be summarized. The data satisfy at high confidence level all the many requirements of the Dark Matter annual modulation signature. Features of the detectors in the field, experimental and theoretical uncertainties, and their implications in the interpretation and comparison of different kinds of results will be discussed as fundamental aspects.
Speaker: Dr Riccardo Cerulli (LNGS)
• 09:55
Dark Matter in the sky 35m
Speaker: Dr Aldo Morselli (INFN Roma II)
• 11:05 11:35
Coffee break 30m Aula B. Touschek, Bldg 36

### Aula B. Touschek, Bldg 36

#### INFN-LNF

Via E. Fermi, 40 00044 Frascati Italy
• 11:35 13:50
Particle dark matter II Aula B. Touschek, Bldg 36

### Aula B. Touschek, Bldg 36

#### INFN-LNF

Via E. Fermi, 40 00044 Frascati Italy
• 11:35
Deeply Inelastic Dark Matter 35m
We examine the production of low mass dark matter particles at the fixed target on the NuMI beamline at Fermilab. Such particles can rescatter in the MINOS near detector producing neutral current-like events. In particular, we bound the couplings of GeV scale Dirac fermion WIMPs for the case that the WIMP-quark interaction is mediated by a (pseudo-)scalar or (axial-)vector which is lighter than the dark matter and compare these bounds to those from old beam dump experiments. We introduce a dipole model to allow the probing of very low mediator masses.
Speaker: Mr Christopher Wallace (IPPP, Durham)
• 12:10
First Direct Detection Limits on sub-GeV Dark Matter and Future Prospects 35m
Direct dark matter (DM) detection experiments almost always focus on Weakly Interacting Massive Particles (WIMPs), which have a mass in the 1--1000 GeV range. However, what if DM is not a WIMP? In this talk, new direct detection strategies for DM particles with MeV to GeV mass will be presented. In this largely unexplored mass range, DM can scatter with electrons, causing ionization of atoms in a detector target material and leading to single- or few-electron events. I will present the first direct detection limits on DM as light as a few MeV, using XENON10 data. Theoretically interesting models can already be probed. Significant improvements in sensitivity should be possible with dedicated experiments, opening up a window to new regions in DM parameter space.
Speaker: Prof. Rouven Essig (Stony Brook University)
• 12:45
Searching for dark matter at the Compact Muon Solenoid experiment 35m
In astrophysical observations, the dark matter is a hypothetical matter which constitutes most of the mass in our universe, but its nature remains unknown. Searches for the dark matter can be divided into three categorized. The first method is to search for the scattered dark matter particles off atomic nuclei within a detector, this method is called the direct detection. The second method is to search for secondary particles such as positrons, antiprotons, or gamma-rays which could originate from annihilations of dark matter particles, this method is called the indirect detection. The last method is to search for dark matter created from the particle collisions at the collider. In this talk, the search for the dark matter at the Large Hadron Collider (LHC) will be presented. The signature has been studied from events containing an energetic jet or photon, and an imbalance in transverse momentum using a data sample of pp collisions at a center-of-mass energy of 7 and 8 TeV. The data has been collected by the Compact Muon Solenoid (CMS) detector at the LHC. Constraints on the dark matter-nucleon scattering cross sections are determined for both spin-independent and spin-dependent interaction models, and compared with results from direct and indirect detections.
Speaker: Dr Norraphat Srimanobhas (Chulalongkorn University, Thailand)
• 13:20
Searches for R-parity conserving supersymmetry with the ATLAS detector 30m
Despite the absence of experimental evidence, weak scale supersymmetry remains one of the best motivated and studied Standard Model extensions. Numerous models of R-parity conserving supersymmetry feature dark matter candidates in form of the lightest neutralino. The ATLAS experiment searches for signs of R-parity conserving supersymmetry in a large variety of signatures involving events with abnormal production of missing transverse momentum, jets, leptons, third generation fermions, gauge bosons or massive long-lived particles. The talk presents a summary of recent results obtained in these searches.
Speaker: Yousuke Kataoka (University of Tokio)
• 13:50 15:20
Lunch break 1h 30m Enea canteen ()

### Enea canteen

• 16:00 17:00
Dark Matter for general public and schools Aula B. Touschek, Bldg 36

### Aula B. Touschek, Bldg 36

#### INFN-LNF

Via E. Fermi, 40 00044 Frascati Italy

Public lecture on dark matter and related searches (in italian).

• 20:00 22:00
Social dinner 2h Rome, Via di Pietra, 89A, +39‐06‐6749701 (La Terrazza del Cesàri)

### Rome, Via di Pietra, 89A, +39‐06‐6749701

#### La Terrazza del Cesàri

Social dinner

• Friday, 19 October
• 09:00 10:10
Dark matter from the cosmos Aula B. Touschek, Bldg 36

### Aula B. Touschek, Bldg 36

#### INFN-LNF

Via E. Fermi, 40 00044 Frascati Italy
• 09:00
CMB as a powerful probe of dark matter annihilation at the epoch of recombination 35m
The injection of secondary particles produced by dark annihilation around redshift 1000 would inevitably affect the process of recombination, leaving an imprint on cosmic microwave background (CMB) temperature and polarization anisotropies. We show that the most recent CMB measurements provided by the WMAP satellite mission and the ACT telescope place interesting constraints on DM self-annihilation rates. Our analysis includes an accurate treatment of the time-dependent coupling of the DM annihilation energy with the thermal gas. We present constraints for specific models of dark matter annihilation channels, as well as a model-independent approach to calculate constraints with future experiments, based on a principal components analysis. We show that current data place already stringent constraints on light DM particles, ruling out thermal WIMPs with mass m < 10GeV annihilating into electrons and WIMPs with mass m < 4GeV annihilating into muons. Finally, we argue that upcoming CMB experiments such as Planck, will improve the constraints by at least 1 order of magnitude, thus providing a sensitive probe of the properties of DM particles.
Speaker: Dr Silvia Galli (IAP)
• 09:35
The dark side of Stars 35m
I will focus on constraints that can be imposed on the properties of dark matter based on observations of neutron stars and white dwarfs. In particular, I will show constraints on WIMP self-interactions (that in some cases are stricter than the bullet cluster) as well as constraints on generic asymmetric dark matter derived from observations of nearby old neutron stars.
Speaker: Prof. Chris kouvaris (CP3-Origins, University of Southern Denmark)
• 10:10 11:20
Future facilities Aula B. Touschek, Bldg 36

### Aula B. Touschek, Bldg 36

#### INFN-LNF

Via E. Fermi, 40 00044 Frascati Italy
• 10:10
Status of Belle II and SuperKEKB 35m
New physics, beyond the standard model, in the quark flavor sector is currently one of the most challenging particle physics topics with tremendous implications in different physics sectors especially if measurements of CP violation in the Standard Model, done at Belle and BaBar experiments, do not explain early universe data like the matter anti-matter asymmetry. With about 40 times more luminosity than KEKB accelerator, SUPERKEKB accelerator and Belle II detector are being built to study such new physics starting in the year 2014-2015. Status of the SUPERKEKB accelerator and status of Belle II detector sub-components will be discussed. Some of B-decay channels with Dark Matter candidates will, also, be discussed within the Belle II detector.
Speaker: Prof. Rachid Ayad (University Of tabuk)
• 10:45
Status of the SuperB project 35m
With an integrated luminosity goal larger than 75 ab-1, the SuperB factory, to be built on the Tor Vergata Campus, near Roma (Italy) by 2016, has the very ambitious goal to unravel the detailed structure of the new physics soon to be discovered at the LHC, or to explore BSM physics beyond the LHC reach if nothing is found there. This goal will be reached using a large number of rare B , charm and tau decays very sensitive to the presence of new heavy particles and dark forces carriers via virtual loops. The physics prospects of this ultra-high luminosity e+e- collider will be presented in detail . The important advantages brought by the specific assets of the SuperB project, especially beam polarization and capability to run at the charm threshold with a significant boost will be presented, with a special emphasis on specific dark forces potential of this new project
Speaker: Riccardo Faccini (ROMA1)
• 11:20 11:50
coffee break 30m Aula B. Touschek, Bldg 36

### Aula B. Touschek, Bldg 36

#### INFN-LNF

Via E. Fermi, 40 00044 Frascati Italy
• 11:50 12:30
Conclusions Aula B. Touschek, Bldg 36

### Aula B. Touschek, Bldg 36

#### INFN-LNF

Via E. Fermi, 40 00044 Frascati Italy
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