Robin Hanson

This paper presents an empirical analysis of the determinants of quantity of health insurance in the context of employer-based health insurance using the micro-level data from the 1987 National Medical Expenditure Survey (NMES). It extends the previous research by including additional factors in the analysis, which significantly affect health insurance offers by employers. This paper emphasizes two determinants of employers’ insurance offer decisions that are particularly relevant: union membership and selfinsured versus not self-insured health plans. The conducted empirical analysis reported in this paper reveals the following predictors of higher health insurance coverage: union membership, not self-insured health plan(s), union membership in Midwest or South, as well as self-insured union membership. Further, other factors such as: age, male, income, for profit and other employer organizational forms, and firm’s size determine a higher level of health insurance.

My horoscope today says, “Focus on the small stuff.” Now, such advice does have content. It predicts that when readers interpret its words in the usual way as a guide to action, those who do what they think it recommends will, on average, feel they got more of what they wanted than those who ignored it. Even so, astrologers sure don’t make it easy for us to test their claims. If they wanted to make it easier, they would do what forecasters in weather, sports, and business do: issue forecasts in a clear, standardized form. A horoscope is like a weather forecast that says, “Some rain likely nearby, soon.” It’s much easier to evaluate a forecast that a particular rain gauge has a..

This paper describes a Bayesian method for constructing a super-resolved surface model by combining information from a set of images of the given surface. We develop the theory and algorithms in detail for the 2-D reconstruction problem, appropriate for the case where all images are taken from roughly the same direction and under similar lighting conditions. We show the results of this 2-D reconstruction on Viking Martian data. These results show dramatic improvements in both spatial and gray-scale resolution. The Bayesian approach uses a neighbor correlation model as well as pixel data from the image set. Some extensions of this method are discussed, including 3-D surface reconstruction and the resolution of diffraction blurred images

Will we have more or fewer deadly wars in the new few decades? Until recently it has been very hard to say much about what makes wars more more frequent or deadly. It doesn't seem to have much to do with levels or changes in population density, whether the economy is booming, how dependent a nation is on trade, or on the number of great powers around. Wars seems only weakly if at all correlated across space and time, seeming for example to be a bit more deadly when they are less frequent. More democratic nations may if anything be more likely to fight wars, though perhaps they less often fight each other, and perhaps join wars more often just after an election [1].

Salop’s “Circular City” model of spatial competition is generalized to higher dimensions, and to “transportation” costs which are a power of distance. Assuming free entry, mill pricing is compared to location-based price discrimination. For dimensions above one, there is some too little entry below some cutoff power, and too much entry above it. This cutoff cost-power rises with dimension, and is larger under price discrimination. Mill pricing induces more entry for powers of four or less, and less entry for powers of five or more. Overall, too much entry seems a more severe problem, which tends to price discrimination

In practice, scoring rules elicit good probability estimates from individuals, while betting markets elicit good consensus estimates from groups. Market scoring rules combine these features, eliciting estimates from individuals or groups, with groups costing no more than individuals. Regarding a bet on one event given another event, only logarithmic versions preserve the probability of the given event. Logarithmic versions also preserve the conditional probabilities of other events, and so preserve conditional independence relations. Given logarithmic rules that elicit relative probabilities of base event pairs, it costs no more to elicit estimates on all combinations of these base events

If we are not to conclude that most planets like Earth have evolved life as intelligent as we are, we must presume Earth is not random. This selection effect, however, also implies that the origin of life need not be as easy as the early appearance of life on Earth suggests. If a series of major evolutionary transitions were required to produce intelligent life, selection implies that a subset of these were “critical steps,” with durations that are similarly distributed. The time remaining from now until simple life is no longer possible on Earth must also be similarly distributed. I show how these results provide timing tests to constrain models of critical evolutionary transitions

Being read is not the same as being believed. Most reviewers have praised the book as original, well-written, thought-provoking, etc., and then gone on to take issue with one or more of Penrose's main theses. Penrose seems unfamiliar with the existing literature in cognitive science, philosophy of mind, and AI. The handful of reviewers who agree with Penrose don't seem to have paid much attention to his specific arguments - they always thought AI was bogus. See, for example, the 37 reviews in Behavioral and Brain Sciences (BBS), Dec. 1990, V13, pp.643-705

In Everett’s many-worlds interpretation, where quantum measurements are seen as decoherence events, inexact decoherence may let large worlds mangle the memories of observers in small worlds, creating a cutoff in observable world measure. I solve a growth–drift–diffusion–absorption model of such a mangled worlds scenario, and show that it reproduces the Born probability rule closely, though not exactly. Thus, inexact decoherence may allow the Born rule to be derived in a many-worlds approach via world counting, using a finite number of worlds and no new fundamental physics

He who pays the piper calls the tune, but he can only succesfully call for a tune that he will recognize upon hearing. Previous models, of two candidates impressing a voter and of firm managers impressing stock speculators, found experts ignoring costly superior information in favor of client preconceptions. Similar result hold when we greatly generalize the agents, choices, information structures, and preferences. When experts must pay to acquire information, have no intrinsic interest in client topics, and can coordinate to acquire the same information, no expert ever pays to know more than any client will know when rewarding those experts

A simple exogenous growth model gives conservative estimates of the economic implications of machine intelligence. Machines complement human labor when they become more productive at the jobs they perform, but machines also substitute for human labor by taking over human jobs. At first, expensive hardware and software does only the few jobs where computers have the strongest advantage over humans. Eventually, computers do most jobs. At first, complementary effects dominate, and human wages rise with computer productivity. But eventually substitution can dominate, making wages fall as fast as computer prices now do. An intelligence population explosion makes per-intelligence consumption fall this fast, while economic growth rates rise by an order of magnitude or more. These results are robust to automating incrementally, and to distinguishing hardware, software, and human capital from other forms of capital

Economic growth is determined by the supply and demand of investment capital; technology determines the demand for capital; while human nature determines the supply. The supply curve has two distinct parts; giving the world economy two distinct modes. In the familiar slow growth mode; rates of return are limited by human discount rates. In the fast growth mode; investment is limited by the world's wealth. Historical trends suggest that we may transition to the fast mode in roughly another century and a half. Can some new technology switch us to the fast mode more quickly than this? Perhaps; but such a technology must greatly raise the rate of return for the world's expected worst investment project. It must thus be very broadly applicable; improving almost all forms of capital and investment. Furthermore; investment externalities must remain within certain limits.

Since utilities and probabilities jointly determine choices, event-dependent utilities complicate the elicitation of subjective event probabilities. However, for the usual purpose of obtaining the information embodied in agent beliefs, it is sufficient to elicit objective probabilities, i.e., probabilities obtained by updating a known common prior with that agent’s further information. Bayesians who play a Nash equilibrium of a certain insurance game before they obtain relevant information will afterward act regarding lottery ticket payments as if they had event-independent risk-neutral utility and a known common prior. Proper scoring rules paid in lottery tickets can then elicit objective probabilities

Attempts to model interstellar colonization may seem hopelessly compromised by uncertainties regarding the technologies and preferences of advanced civilizations. If light speed limits travel speeds, however, then a selection effect may eventually determine frontier behavior. Making weak assumptions about colonization technology, we use this selection effect to predict colonists’ behavior, including which oases they colonize, how long they stay there, how many seeds they then launch, how fast and far those seeds fly, and how behavior changes with increasing congestion. This colonization model explains several astrophysical puzzles, predicting lone oases like ours, amid large quiet regions with vast unused resources.

Consider a health policy issue like child car seats in the U.S., mosquito netting in the third world, preschool education for poor children, or the immunization of immigrants. Imagine that for this issue there were many good studies over several decades, including some recent studies. Imagine that after controlling for many factors, these studies usually found that variations in spending or usage were significantly, substantially, and positively related to variations in health. Furthermore, imagine this result was confirmed by a thirty year old randomized experiment.

In their article, ‘That is not dead which can eternal lie: the aestivation hypothesis for resolving Fermi’s paradox’, Sandberg et al. try to explain the Fermi paradox by claiming that Landauer’s principle implies that a civilization can in principle perform far more times more) irreversible logical operations if it conserves its resources until the distant future when the cosmic background temperature is very low. So perhaps aliens are out there, but quietly waiting. Sandberg et al. implicitly assume, however, that computer-generated entropy can only be disposed of by transferring it to the cosmological background. In fact, while this assumption may apply in the distant future, our universe today contains vast reservoirs and other physical systems in non-maximal entropy states, and computer-generated entropy can be transferred to them at the adiabatic conversion rate of one bit of negentropy to erase one bit of error. This can be done at any time, and is not improved by waiting for a low cosmic background temperature. Thus aliens need not wait to be active. As Sandberg et al. do not provide a concrete model of the effect they assert, we construct one and show where their informal argument goes wrong.

Are you fascinated by some basic questions about science, technology, and our future? Questions like: Is cryonics technically feasible? When will nano‐assemblers be feasible and how quickly will resulting changes come? Does a larger population help or hinder the world environment and economy? Will uploading be possible, and if so when? When can I live in space? Where will I be able to live free from tyranny? When will AIs be bucking for my job? Is there intelligent life beyond earth? If you are like most Extropy readers, such questions matter to you.

This chapter assesses realistic social implications of emulation (em). It takes the somewhat unusual approach of using basic social theory, in addition to common sense and trend projection, to forecast future societies. Em cities are likely toxic to ordinary humans, who, controlling most of the rest of the Earth, mostly live comfortably on their em‐economy investments. Em's extended lifespans induce greater wealth inequality among ems. Ems focus their identity less on individual personalities and abilities, and more on being part of a particular team. While copy clans coordinate to show off common clan abilities, individual ems focus on showing their identities, abilities, and loyalties as team players. The analysis in this chapter suggests that lives in the next great era might be as different from what we are accustomed to as ours are from farmers' lives, or farmers' from foragers'.

Purpose This paper aims to formalize long-term trajectories of human civilization as a scientific and ethical field of study. The long-term trajectory of human civilization can be defined as the path that human civilization takes during the entire future time period in which human civilization could continue to exist. Design/methodology/approach This paper focuses on four types of trajectories: status quo trajectories, in which human civilization persists in a state broadly similar to its current state into the distant future; catastrophe trajectories, in which one or more events cause significant harm to human civilization; technological transformation trajectories, in which radical technological breakthroughs put human civilization on a fundamentally different course; and astronomical trajectories, in which human civilization expands beyond its home planet and into the accessible portions of the cosmos. Findings Status quo trajectories appear unlikely to persist into the distant future, especially in light of long-term astronomical processes. Several catastrophe, technological transformation and astronomical trajectories appear possible. Originality/value Some current actions may be able to affect the long-term trajectory. Whether these actions should be pursued depends on a mix of empirical and ethical factors. For some ethical frameworks, these actions may be especially important to pursue.

Compared with non-union workers, union workers take more of their compensation in the form of insurance. This may be because unions choose democratically, and democratic choice mitigates adverse selection in group insurance. Relative to individually-purchased insurance, we show that group insurance chosen by an ideal profit-maximizing employer can be worse for every employee, while group insurance chosen democratically can be much better. The reason is that democracy can fail to represent the preferences of almost half the group

The ability to inject dopant atoms with high spatial resolution, flexibility in dopant species, and high single ion detection fidelity opens opportunities for the study of dopant fluctuation effects and the development of devices in which function is based on the manipulation of quantum states in single atoms, such as proposed quantum computers. The authors describe a single atom injector, in which the imaging and alignment capabilities of a scanning force microscope are integrated with ion beams from a series of ion sources and with sensitive detection of current transients induced by incident ions. Ion beams are collimated by a small hole in the SFM tip and current changes induced by single ion impacts in transistor channels enable reliable detection of single ion hits. They discuss resolution limiting factors in ion placement and processing and paths to single atom array formation for systematic testing of quantum computer architectures in silicon and diamond. © 2008 American Vacuum Society.