NAFTA and the Mexican Economy

The North American Free Trade Agreement (NAFTA), in effect since January 1994, plays a very strong role in the bilateral economic relationship between Mexico and the United States. The two countries are also closely tied in areas not directly related to trade and investment such as security, environmental, migration, and health issues. The effects of NAFTA on Mexico and the state of the Mexican economy have important impacts on U.S. economic and political interests. As NAFTA approaches its 15th anniversary, a number of policymakers have raised the issue of revisiting NAFTA and renegotiating parts of the agreement. Some important factors in evaluating NAFTA include the effects of the agreement on Mexico and how these relate to U.S.-Mexico economic relations. In the 110th Congress, major issues of concern have been related mostly to economic conditions in Mexico, the effect of NAFTA on the United States and Mexico, and Mexican migrant workers in the United States. In 1990, then Mexican President Carlos Salinas de Gortari approached the United States with the idea of forming a free trade agreement (FTA). Mexico’s main motivation in pursuing an FTA with the United States was to stabilize the Mexican economy by attracting foreign direct investment. The Mexican economy had experienced many difficulties throughout most of the 1980s with a significant deepening of poverty. The intention of Mexico in entering NAFTA was to increase export diversification by attracting foreign direct investment (FDI), which would help create jobs, increase wage rates, and reduce poverty. At the time that NAFTA went into effect, the expectation among supporters was that the agreement would improve investor confidence in Mexico, attract investment, and narrow the income differentials between Mexico and the United States and Canada. Measuring the effects of NAFTA on the Mexican economy is difficult because the economy was also affected by other factors, such as economic cycles in the United States (Mexico’s largest trading partner) and currency fluctuations. In addition, Mexico’s unilateral trade liberalization measures of the 1980s and the currency crisis of 1995 both affected economic growth, per capita gross domestic product (GDP), and real wages. While NAFTA may have brought economic and social benefits to the Mexican economy as a whole, the benefits have not been evenly distributed throughout the country. Wages and employment tend to be higher in states experiencing higher levels of FDI and trade. The agricultural sector experienced a higher amount of worker displacement after NAFTA because of increased competition from the United States and because of Mexican domestic agricultural reforms. In terms of regional effects, initial conditions in Mexico determined which Mexican states experienced stronger economic growth as a result of NAFTA. States with higher levels of telecommunications and transportation infrastructure gained more benefits than poorer states with lower levels of education, infrastructure, and institutional capacity. Some economists argue that while trade liberalization may narrow income disparities over the long run with other countries, it may indirectly lead to larger disparities in income levels within a country. This report will be updated as events warrant

The feminine face of Science

Uno de los objetivos fijados en la asignatura Ciencias para el mundo contemporáneo (1º de Bachillerato) es el de superar el escaso interés que siente el alumnado hacia la ciencia. Es necesario para tal fin un cambio en los planteamientos tanto metodológicos como temáticos, respecto a las asignaturas de ciencias tradicionales. Con la intención de contribuir a este cambio se han diseñado actividades en las que confluyen características que podrán ayudar a conseguirlo. En el caso propuesto se escogió una temática controvertida a lo largo de la historia: Mujeres y Ciencia; eligiendo como estrategia de aprendizaje las webquests y publicando en la red las tareas realizadas por el alumnado, todo esto con la finalidad de romper las paredes del aula y hacer extensiva la cultura científica al resto de la comunidad educativa y público en general

Nonminimal Inflation on the Randall-Sundrum II Brane with Induced Gravity

We study an inflation model that inflaton field is non-minimally coupled to the induced scalar curvature on the Randall-Sundrum (RS) II brane. We investigate the effects of the non-minimal coupling on the inflationary dynamics of this braneworld model. Our study shows that the number of e-folds decreases by increasing the value of the non-minimal coupling. We compare our model parameters with the minimal case and also with recent observational data. In comparison with recent observation, we obtain a constraint on the values that the non-minimal coupling attains.Comment: 15 pages, 5 figure

Control of fluorescence in quantum emitter and metallic nanoshell hybrids for medical applications

We study the light emission from quantum emitter and double metallic nanoshell hybrid systems. Quantum emitters act as local sources which transmit their light efficiently due to a double nanoshell near field. The double nanoshell consists a dielectric core and two outer nanoshells

Retired galaxies: not to be forgotten in the quest of the star formation -- AGN connection

We propose a fresh look at the Main Galaxy Sample of the Sloan Digital Sky Survey by packing the galaxies in stellar mass and redshift bins. We show how important it is to consider the emission-line equivalent widths, in addition to the commonly used emission-line ratios, to properly identify retired galaxies (i.e. galaxies that have stopped forming stars and are ionized by their old stellar populations) and not mistake them for galaxies with low-level nuclear activity. We find that the proportion of star-forming galaxies decreases with decreasing redshift in each mass bin, while that of retired galaxies increases. Galaxies with $M_\star > 10^{11.5} M_\odot$ have formed all their stars at redshift larger than 0.4. The population of AGN hosts is never dominant for galaxy masses larger than $10^{10} M_\odot$. We warn about the effects of stacking galaxy spectra to discuss galaxy properties. We estimate the lifetimes of active galactic nuclei (AGN) relying entirely on demographic arguments --- i.e. without any assumption on the AGN radiative properties. We find upper-limit lifetimes of about 1--5 Gyr for detectable AGN in galaxies with masses between $10^{10}$--$10^{12} M_\odot$. The lifetimes of the AGN-dominated phases are a few $10^8$ yr. Finally, we compare the star-formation histories of star-forming, AGN and retired galaxies as obtained by the spectral synthesis code STARLIGHT. Once the AGN is turned on it inhibits star formation for the next $\sim$ 0.1 Gyr in galaxies with masses around $10^{10} M_\odot$, $\sim$ 1 Gyr in galaxies with masses around $10^{11} M_\odot$.Comment: accepted for MNRAS figure resolution has been degraded with respect to what will be published in MNRA

Topological defects and misfit strain in magnetic stripe domains of lateral multilayers with perpendicular magnetic anisotropy

Stripe domains are studied in perpendicular magnetic anisotropy films nanostructured with a periodic thickness modulation that induces the lateral modulation of both stripe periods and inplane magnetization. The resulting system is the 2D equivalent of a strained superlattice with properties controlled by interfacial misfit strain within the magnetic stripe structure and shape anisotropy. This allows us to observe, experimentally for the first time, the continuous structural transformation of a grain boundary in this 2D magnetic crystal in the whole angular range. The magnetization reversal process can be tailored through the effect of misfit strain due to the coupling between disclinations in the magnetic stripe pattern and domain walls in the in-plane magnetization configuration