Income redistribution: how to divide the pie?

In this paper, we elicit preferences of Swiss citizens for the allocation of income redistribution to different uses through a Discrete Choice Experiment performed in 2008. Neustadt and Zweifel (2009} provide an estimate of the total desired amount of income redistribution as a share of disposable income. Here, we estimate marginal willingness-to-pay values for types of recipients (old-age pensioners, people with ill health, the unemployed, working poor, and families with children) and their nationality (Swiss, citizens of western European countries, others). Hypotheses derived from the insurance motive for redistribution receive some empirical support.Income redistribution, preferences, willingness to pay, discrete choice experiments, conjoint analysis, social status

Is the Welfare State Sustainable? Experimental Evidence on Citizens' Preferences for Redistribution

The sustainability of the welfare state ultimately depends on citizens' preferences for income redistribution. They are elicited through a Discrete Choice Experiment performed in 2008 in Switzerland. Attributes are redistribution as GDP share, its uses (the unemployed, old-age pensioners, people with ill health etc.), and nationality of beneficiary. Estimated marginal willingness to pay (WTP) is positive among those who deem benefits too low, and negative otherwise. However, even those who state that government should reduce income inequality exhibit a negative WTP on average. The major finding is that estimated average WTP is maximum at 21% of GDP, clearly below the current value of 25%. Thus, the present Swiss welfare state does not appear sustainable.Income redistribution; welfare state; sustainability; preferences; willingness to pay; discrete choice experiments

Economic Well-Being, Social Mobility, and Preferences for Income Redistribution: Evidence from a Discrete Choice Experiment

In this paper, preferences for income redistribution in Switzerland are elicited through a Discrete Choice Experiment (DCE) performed in 2008. In addition to the amount of redistribution as a share of GDP, attributes also included its uses (working poor, the unemployed, old-age pensioners, families with children, people in ill health) and nationality of beneficiary (Swiss, Western European, others). Willingness to pay for redistribution increases with income and education, contradicting the conventional Meltzer-Richard (1981) model. The Prospect of Upward Mobility hypothesis [Hirschman and Rothschild (1973); Benabou and Ok (2001)] receives partial empirical support.Income redistribution, preferences, willingness to pay, discrete choice experiments, stated choice, economic well-being, social mobility

Asteroid Belt Meteoroid Hazard Study

Mathematical models for probability of successful traverse of asteroid belt or zero penetration of spacecraft shiel

Discovery of an Apparent High Latitude Galactic Supernova Remnant

Deep H$\alpha$ images of a faint emission complex 4.0 x 5.5 degrees in angular extent and located far off the Galactic plane at l = 70.0 degrees, b=-21.5 degrees reveal numerous thin filaments suggestive of a supernova remnant's shock emission. Low dispersion optical spectra covering the wavelength range 4500 - 7500 A show only Balmer line emissions for one filament while three others show a Balmer dominated spectrum along with weak [N I] 5198, 5200 A, [O I] 6300, 6364 A, [N II] 6583 A, [S II] 6716, 6731 A and in one case [O III] 5007 A line emission. Many of the brighter H$\alpha$ filaments are visible in near UV GALEX images presumably due to C III] 1909 A line emission. ROSAT All Sky Survey images of this region show a faint crescent shaped X-ray emission nebula coincident with the portion of the H$\alpha$ nebulosity closest to the Galactic plane. The presence of long, thin Balmer dominated emission filaments with associated UV emission and coincident X-ray emission suggests this nebula is a high latitude Galactic supernova remnant despite a lack of known associated nonthermal radio emission. Relative line intensities of the optical lines in some filaments differ from commonly observed [S II]/H$\alpha$ > 0.4 radiative shocked filaments and typical Balmer filaments in supernova remnants. We discuss possible causes for the unusual optical SNR spectra.Comment: 12 pages, 10 figures, accepted to the Astrophysical Journa

Border Songs: Bringing the Immigration Crisis to the Classroom with Music

During fall semester of 2010, I began taking students on five-day field trips to the Arizona–Mexico border. One part of these trips involves meeting with sound sculptor Glenn Weyant, who plays the border wall as a musical instrument. Weyant attaches contact microphones to the wall and plays it, sometimes bowing the steel structure with a cello bow, and other times playing it rhythmically with what he calls “instruments of mass percussion.

Reading Spanish American national anthems: “Sonograms” of national identity

Analysis of the text, music, and historical development of representative Spanish American national anthems. Primarily concentrating on the Chilean and Costa Rican himnos nacionales