The Semi-Hooperon: Gamma-ray and anti-proton excesses in the Galactic Center

A puzzling excess in gamma-rays at GeV energies has been observed in the center of our galaxy using Fermi-LAT data. Its origin is still unknown, but it is well fitted by Weakly Interacting Massive Particles (WIMPs) annihilations into quarks with a cross section around $10^{-26}{\rm cm^3 s^{-1}}$ with masses of $20-50$~GeV, scenario which is promptly revisited. An excess favoring similar WIMP properties has also been seen in anti-protons with AMS-02 data potentially coming from the Galactic Center as well. In this work, we explore the possibility of fitting these excesses in terms of semi-annihilating dark matter, dubbed as semi-Hooperon, with the process ${\rm WIMP\, WIMP \rightarrow WIMP\, X}$ being responsible for the gamma-ray excess, where X=h,Z. An interesting feature of semi-annihilations is the change in the relic density prediction compared to the standard case, and the possibility to alleviate stringent limits stemming from direct detection searches. Moreover, we discuss which models might give rise to a successful semi-Hooperon setup in the context of $\mathcal{Z}_3$,$\mathcal{Z}_4$ and extra "dark" gauge symmetries.Comment: 8 pages, 3 figures, version published in Phys. Lett.

Fractional Brownian motions ruled by nonlinear equations

In this note we consider generalized diffusion equations in which the diffusivity coefficient is not necessarily constant in time, but instead it solves a nonlinear fractional differential equation involving fractional Riemann-Liouville time-derivative. Our main contribution is to highlight the link between these generalised equations and fractional Brownian motion (fBm). In particular, we investigate the governing equation of fBm and show that its diffusion coefficient must satisfy an additive evolutive fractional equation. We derive in a similar way the governing equation of the iterated fractional Brownian motion.Comment: 7 page

Does Microcredit Reach the Poor and Vulnerable? Evidence from Northern Bangladesh

Subsidized loans have a history of being diverted to the rich. Yet recently microcredit programs, such as the Grameen Bank in Bangladesh, have become popular among donors and governments as a way to channel funds to the poor. This paper uses a unique panel dataset from two Bangladeshi villages to test if the modern microcredit movement is different from its predecessors. Poverty is measured by levels of consumption. Vulnerability is measured as fluctuations in consumption associated with inefficient risk sharing. We find that subsidized credit is largely successful at reaching the poor and vulnerable. The probability that a microcredit member is below the poverty line is substantially higher than that of a randomly picked household in both villages. In the village where female headed households were found to be vulnerable, nearly half of the female headed households belonged to microcredit programs yet only a quarter of male headed households were microcredit members. While restricting loans to the landless is not effective in reaching the poor and vulnerable, targeting female headed households is.

Monetary Policy Rules, Asset Prices and Exchange Rates

We examine empirically whether asset prices and exchange rates may be admitted into a standard interest rate rule, using data for the US, the UK and Japan since 1979. Asset prices and exchange rates can be employed as information variables for a standard ‘Taylor-type’ rule or as arguments in an augmented interest rate rule. Our empirical evidence, based on measures of the output gap proxied by marginal costs calculations, suggests that monetary policy-makers may use asset prices and exchange rates not only as part of their information set for setting interest rates, but also to set interest rates to offset deviations of asset prices or exchange rates from their equilibrium levels. These results are open to several alternative interpretations.Asset prices; exchange rates; interest rate rules; monetary policy.

Pseudoscalar Mediators: A WIMP model at the Neutrino Floor

Due to its highly suppressed cross section (fermionic) dark matter interacting with the Standard Model via pseudoscalar mediators is expected to be essentially unobservable in direct detection experiments. We consider both a simplified model and a more realistic model based on an extended two Higgs doublet model and compute the leading one-loop contribution to the effective dark matter- nucleon interaction. This higher order correction dominates the scattering rate completely and can naturally, i.e. for couplings of order one, lead to a direct detection cross section in the vicinity of the neutrino floor. Taking the observed relic density and constraints from low-energy observables into account we analyze the direct detection prospects in detail and find regions of parameter space that are within reach of upcoming direct detection experiments such as XENONnT, LZ, and DARWIN.Comment: 29 pages, 8 figure

A first principle computation of the thermodynamics of glasses

We propose a first principle computation of the equilibrium thermodynamics of simple fragile glasses starting from the two body interatomic potential. A replica formulation translates this problem into that of a gas of interacting molecules, each molecule being built of m atoms, and having a gyration radius (related to the cage size) which vanishes at zero temperature. We use a small cage expansion, valid at low temperatures, which allows to compute the cage size, the specific heat (which follows the Dulong and Petit law), and the configurational entropy.Comment: Latex, 40 pages, 9 figures, corrected misprints, improved presentatio

Augury of Darkness: The Low-Mass Dark Z' Portal

Dirac fermion dark matter models with heavy $Z^{\prime}$ mediators are subject to stringent constraints from spin-independent direct searches and from LHC bounds, cornering them to live near the $Z^{\prime}$ resonance. Such constraints can be relaxed, however, by turning off the vector coupling to Standard Model fermions, thus weakening direct detection bounds, or by resorting to light $Z^{\prime}$ masses, below the Z pole, to escape heavy resonance searches at the LHC. In this work we investigate both cases, as well as the applicability of our findings to Majorana dark matter. We derive collider bounds for light $Z^{\prime}$ gauge bosons using the $CL_S$ method, spin-dependent scattering limits, as well as the spin-independent scattering rate arising from the evolution of couplings between the energy scale of the mediator mass and the nuclear energy scale, and indirect detection limits. We show that such scenarios are still rather constrained by data, and that near resonance they could accommodate the gamma-ray GeV excess in the Galactic center.Comment: 25 pages, 6 Figures. Typos correcte