We study the response of a uniformly accelerated model particle detector in a spacetime with compact spatial sections. The basic thermal character of the response re-emerges, in spite of the fact that the spacetime does not possess event horizons. Our model also permits a study of detector response to twisted field states.

It has been shown by Gupta and Padmanabhan that the radiation reaction force of the Abraham–Lorentz–Dirac equation can be obtained by a coordinate transformation from the inertial frame of an accelerating charged particle to that of the laboratory. We show that the problem may be formulated in a flat space of five dimensions, with five corresponding gauge fields in the framework of the classical version of a fully gauge covariant form of the Stueckelberg–Feynman–Schwinger covariant mechanics (the zero mode (...) fields of the 0, 1, 2, 3 components correspond to the Maxwell fields). Without additional constraints, the particles and fields are not confined to their mass shells. We show that in the mass-shell limit, the generalized Lorentz force obtained by means of the retarded Green's functions for the five dimensional field equations provides the classical Abraham–Lorentz–Dirac radiation reaction terms (with renormalized mass and charge). We also obtain general coupled equations for the orbit and the off-shell dynamical mass during the evolution as well as an autonomous non-linear equation of third order for the off-shell mass. The theory does not admit radiation if the particle does not move off-shell. The structure of the equations implies that mass-shell deviation is bounded when the external field is removed. (shrink)

We argue that purely local experiments can distinguish a stationary charged particle in a static gravitational field from an accelerated particle in (gravity-free) Minkowski space. Some common arguments to the contrary are analyzed and found to rest on a misidentification of “energy.”.

The conditions in which electromagnetic radiation is formed are discussed. It is found that the main condition for the emission of radiation by an electric charge is the existence of a relative acceleration between the charge and its electric field. Such a situation exists both for a charge accelerated in a free space, and for a charge supported at rest in a gravitational field. Hence, in such situations, the charges radiate. It is also shown that relating (...) class='Hi'>radiation to the relative acceleration between a charge and its electric field, solves several difficulties that existed in earlier approaches, like the “energy balance paradox,” and the “relativistic” nature of the observation of the emitted radiation. (shrink)

It is suggested that an understanding of blackbody radiation within classical physics requires the presence of classical electromagnetic zero-point radiation, the restriction to relativistic (Coulomb) scattering systems, and the use of discrete charge. The contrasting scaling properties of nonrelativistic classical mechanics and classical electrodynamics are noted, and it is emphasized that the solutions of classical electrodynamics found in nature involve constants which connect together the scales of length, time, and energy. Indeed, there are analogies between the electrostatic forces (...) for groups of particles of discrete charge and the van der Waals forces in equilibrium thermal radiation. The differing Lorentz- or Galilean-transformation properties of the zero-point radiation spectrum and the Rayleigh-Jeans spectrum are noted in connection with their scaling properties. Also, the thermal effects of acceleration within classical electromagnetism are related to the existence of thermal equilibrium within a gravitational field. The unique scaling and phase-space properties of a discrete charge in the Coulomb potential suggest the possibility of an equilibrium between the zero-point radiation spectrum and matter which is universal (independent of the particle mass), and an equilibrium between a universal thermal radiation spectrum and matter where the matter phase space depends only upon the ratio mc 2/k B T. The observations and qualitative suggestions made here run counter to the ideas of currently accepted quantum physics. (shrink)

The law of gravitation is taken in the formR 44=0, whereR 44 is the time curvature component of the Ricci tensor. Space-time separable equations are developed in spherical coordinates for the nonlinear wave equation determined byR 44=0. One exact solution is examined in detail.

In lieu of an abstract, here is a brief excerpt of the content:Fallout from Government-Sponsored Radiation ResearchCarol Mason Spicer (bio)On December 28, 1993, Energy Secretary Hazel R. O'Leary publicly appealed to both the executive and legislative branches of the United States Government to consider compensation for individuals who were harmed by their exposure to ionizing radiation while enrolled in government-sponsored studies conducted between 1940 and the early 1970s.1 The call for compensation was issued three weeks after Secretary O'Leary (...) disclosed that radiation experiments involving humans, sometimes without their consent, had occurred under the auspices of the Atomic Energy Commission (AEC), a forerunner of the Department of Energy (DOE). Secretary O'Leary directed her department to investigate the nature and extent of the experiments, report on their medical and ethical acceptability, and locate the research subjects or their families.Background to the Federal Advisory CommitteeDespite the fact that the existence of many government-sponsored radiation experiments was not a secret—much of the research was reported at the time in scientific journals, and in 1986, Representative Edward J. Markey (D-MA) conducted congressional hearings on such radiation research—Secretary O'Leary's disclosure of the AEC experiments and her call for compensation made the experiments common knowledge and sparked a swift and complex governmental response involving both the executive and legislative branches.It is curious that the "radiation experiments" have garnered so much attention now, since they were virtually ignored in the wake of the 1986 hearings. Secretary O'Leary's disclosure of the radiation studies grew out of a general reassessment of secrecy in government. In April 1993, the Clinton administration set out to review the system of government secrecy that evolved during the Cold War, and in May 1993, DOE began reviewing and declassifying files pertaining to nuclear weapons research. When Dan Reicher, a top aide to Secretary O'Leary, informed her in November of the impending publication of an Albuquerque Tribune investigative report (Welsome 1993) on an experiment conducted between 1945 and 1947 in which 18 subjects were injected with plutonium, [End Page 147] the topic of questionable research involving the exposure of human subjects to radiation was added to the DOE list of information to be disclosed. At the time, it was thought to be but one small part of a massive quantity of DOE information to be made public.As part of its effort to investigate the radiation experiments, DOE established a toll-free telephone hot line for individuals who thought they might have been the subjects of radiation exposure experiments. The hot line, originally staffed by three people to handle the anticipated few dozen calls per day, received more than 2,000 calls in the first week. By early January the hot line was flooded with 6,000 to 10,000 calls daily, and its staff had increased more than ten-fold. Although many of the calls were deemed not to be candidates for further investigation, the extent of the radiation-related experiments, sponsored not only by AEC, but also by the military and other government departments and agencies, took officials by surprise.On December 30, the Department of Defense, the Department of Veterans Affairs, and the National Aeronautics and Space Administration all announced that they were initiating thorough reviews of their files to determine the extent and nature of any radiation experiments conducted under their auspices.2 In January, the CIA and the Department of Health and Human Services, including the National Institutes of Health, followed suit.The White House publicly entered the arena in late December announcing that it would hold a meeting on January 3, 1994, to help coordinate the government's investigative effort. At the same time, Senator Edward M. Kennedy (D-MA) called for a mid-January congressional hearing to investigate experiments conducted between 1946 and 1956 in which mentally retarded boys at the Fernald State School in Massachusetts were fed radioactive iron supplements or milk containing radioactive calcium to enable researchers to trace the absorption of those nutrients. Senator Kennedy's hearing, conducted by the Subcommittee on Health of the Senate Committee on Labor and Human Resources, was the first of a number of congressional hearings held earlier this year to investigate the... (shrink)

“In space”, declared the posters for the 1979 movie Alien, in a deliberately disconcerting juxtaposition, “no-one can hear you scream.” Yet even the space that lies beyond the earth is not utterly silent – stars and planets themselves produce sounds that radiate through the rarefied gases lying between them, although the wavelengths produced lie far beyond the range of human hearing. There are, then, not even in the spaces between the planets and the stars, any truly silent spaces, (...) and merely to be present in a space, no matter the nature of the space in question, is already to disturb that space in multiple ways – such disturbance typically being manifest acoustically no less than visually. Yet often we tend to conceptualise space and spatial presence in terms that actually give priority to the visual over the acoustic, and even to neglect the spatial character of the acoustic altogether. A classic example of this is to be found in the work of the British philosopher Peter Strawson who famously proposed, as a kind of thought-experiment, the idea of what he called a ‘No-Space world’ that was constituted in purely auditory terms, and was for just this reason taken to be a non-spatial world. 1.. (shrink)

This paper aims to argue for the thesis that it is not a priori morally justified that the first phase of space colonisation is based on sexual reproduction. We ground this position on the argument that, at least in the first colonisation settlements, those born in space may not have a good chance of having a good life. This problem does not depend on the fact that life on another planet would have to deal with issues such as (...) solar radiation or with the decrease or entire absence of the force of gravity. These issues could plausibly be addressed given that the planets or settlements we will feasibly colonise could be completely transformed through geoengineering processes. Likewise, the ability of humans to live in space could be enhanced through genetic modification interventions. Even if, however, the problems concerning survival in space were solved, we think that, at least in the first period of colonisation of space or other planets, giving birth to children in space could be a morally irresponsible choice since we argue, the life we ​​could give them might not be good enough. We contend that this is the case since when we decide to have a baby. We argue that it is not morally right to be content that our children have a minimally sufficient life worth living; before we give birth to children in space, we should make sure we can give them a reasonable chance of having a good life. This principle applies both on Earth - at least where you can choose - and for space travel. (shrink)

Space is one of the most fundamental concepts over which scientific knowledge has been constructed. But it is also true that space concepts extrapolate by far the scientific domain, and permeate many other branches of human knowledge. Those are fascinating aspects that could di per se justify the compilation of a long bibliography. Another one is the passion for books. My interest in some physical, historical and philosophical problems concerning the concept of space in Physics, and its (...) properties, can be traced back to the early 1980. Since that time, I have being studying, with several collaborators, the influence of space dimensionality in different physical phenomena, like the Casimir Effect, neutron diffraction, Cosmic Microwave Background Radiation and the stability of Schrödinger’s and Dirac’s hydrogen atom in arbitrary number of dimensions, as well as epistemological aspects of the works of Kant, Ehrenfest an others on this particular subject. Meanwhile, I gave lectures about the History of the Concepts of Space in Physics at the Centro Brasileiro de Pesquisas Físicas (CBPF), at the Program of History of Sciences, Technics and Epistemology of the Federal University of Rio the Janeiro (UFRJ) and also at the Physics Institute of the State University of Rio de Janeiro (UERJ). As a consequence of both this interest and my love for books, I continuously bought books on space for my personal library which contains now quite one half of all the books quoted here. In 1996, Roberto Moreira and I published the Sources for the History of Space concepts in Physics: From 1845 to 1995 in the series Notas de Física of the CBPF (NF # 084/96), which is still available online. This was a first initiative to share our bibliography on space. At that time, it contained 1075 references, including 414 books entirely devoted to space, 380 articles in periodical journals and proceedings and 281 miscellaneous citations. After fifteen years, I decided to focus my attention here to collect what in my opinion are the 601 essential books which could be useful for anyone interested on learning about space. An important restriction is imposed here by language: only texts written in English, French, German, Italian, Spanish, Portuguese and Latin were considered. References are given in chronological order covering the period between 1739 and 2010. For each year, the books are listed in alphabetical order of authors’ name. An onomastic index is included at the end of the book. -/- Francisco Caruso Rio de Janeiro, October 2011 . (shrink)

In addition to double‐ and single‐strand DNA breaks and isolated base modifications, ionizing radiation induces clustered DNA damage, which contains two or more lesions closely spaced within about two helical turns on opposite DNA strands. Post‐irradiation repair of single‐base lesions is routinely performed by base excision repair and a DNA strand break is involved as an intermediate. Simultaneous processing of lesions on opposite DNA strands may generate double‐strand DNA breaks and enhance nonhomologous end joining, which frequently results in the (...) formation of deletions. Recent studies support the possibility that the mechanism of base excision repair contributes to genome stability by diminishing the formation of double‐strand DNA breaks during processing of clustered lesions. BioEssays 23:745–749, 2001. © 2001 John Wiley & Sons, Inc. (shrink)

Radioactivity accompanied by ionizing radiation has always existed on the Earth, as well as in space, and so in every living tissue there are traces of radioactivity. With the discovery of the said radiation and identifying its effects on the human body, the fear of this phenomenon appeared. At high doses radiation causes serious tissue damages, while at small doses it can cause cancer and induce genetic defects. The best antidote for fear is knowledge. It is (...) important to know the margins safety of radiation for human life. As a result, the topic of radioactive contamination of the environment has now become one of the most significant. In recent years the radon problem is a subject of a wide debate of geologists, geophysicists, ecologists, physicians, specialists in radiometry, and, of course, philosophers and sociologists, since the need for assessing the potential radon danger concerns human lives, human functions in society, and human future. (shrink)

While humans have made enormous progress in the exploration and exploitation of Earth, exploration of outer space remains beyond current human capabilities. The principal challenges lie in current space technology and engineering which includes the protection of astronauts from the hazards of working and living in the space environment. These challenges may lead to a paradoxical situation where progress in space technology and the ability to ensure acceptable risk/benefit for human space exploration becomes dissociated and (...) the rate of scientific discovery declines. In this paper, we discuss the predominant challenges of the space environment for human health and argue that development and deployment of a human enhancement policy, initially confined to astronauts – for the purpose of future human space programmes is a rational solution to these challenges. (shrink)

This paper uses a novel account of non-ideal political action that can justify radical responses to severe climate injustice, including and especially deliberate attempts to engineer the climate system in order reflect sunlight into space and cooling the planet. In particular, it discusses the question of what those suffering from climate injustice may do in order to secure their fundamental rights and interests in the face of severe climate change impacts. Using the example of risky geoengineering strategies such as (...) sulfate aerosol injections, I argue that peoples that are innocently subject to severely negative climate change impacts may have a special permission to engage in large-scale yet risky climate interventions to prevent them. Furthermore, this can be true even if those interventions wrongly harm innocent people. (shrink)

In lieu of an abstract, here is a brief excerpt of the content:Chair’s Perspective on the Work of the Advisory Committee on Human Radiation ExperimentsRuth Faden (bio)On January 15, 1994, President Clinton created the Advisory Committee on Human Radiation Experiments in response to his concern about the increasing number of reports describing alleged unethical conduct of the U.S. Government, and institutions funded by the government, in the use of, or exposure to, ionizing radiation in human beings at (...) the height of the Cold War. He directed the Committee: (1) to uncover the history of human radiation experiments and intentional environmental releases of radiation; (2) to identify the ethical and scientific standards for evaluating these events; and (3) to make recommendations to ensure that whatever wrongdoing may have occurred in the past will not be repeated.The Committee was composed of 14 members: a citizen representative and 13 experts in bioethics, radiation oncology and biology, epidemiology and statistics, public health, history of science and medicine, nuclear medicine, and law. We reported to a cabinet-level group (the Human Radiation Interagency Working Group) convened by the president, which includes the secretaries of defense, energy, health and human services, and veterans affairs; the attorney general; the administrator of the National Aeronautics and Space Administration; the director of the Central Intelligence Agency; and the director of the Office of Management and Budget.On April 21, 1994, at the end of the first day of our first meeting, President Clinton invited us to the White House to personally communicate his commitment to the process we were about to undertake. He urged us to be fair, thorough, and unafraid to shine the light of truth on this hidden and poorly understood aspect of our nation’s past. Our most important task, he said, was to tell the full story to the American public. [End Page 215] At the same time, we were to examine the present, to determine how the conduct of human research today compares with that of the past, and to assess whether, in light of this inquiry, changes need to be made in the policies of the federal government. Eighteen months later, the Committee’s attempt to tell the story of the past and to report on our inquiry into the present was delivered to the president in a 900-page Final Report (ACHRE 1995) and several supplemental volumes.The Committee’s charge was enormous. We were asked to conduct a massive investigation into events that occurred as much as 50 years ago and that involved the highest reaches of the defense establishment and the medical community. This investigation necessitated an examination of the conduct and policies of six federal agencies and countless agents in the private sector, as well as the location and interpretation of hundreds of thousands of documents, many of which were buried in obscure locations or were still classified.In addition, the Committee was instructed to establish standards for judging, in moral terms, the events that it uncovered. This charge necessitated the confrontation of contentious debates in moral thought and theory about history, relativism, and the significance of context in moral judgment. But our purpose was not to engage in these debates in the abstract. Although the Committee was not expressly charged with considering issues relating to remedies, including financial compensation, we felt obliged to address the type of remedies that we believed the government, as an ethical matter, should provide to subjects of experiments where the circumstances warranted such a response. Thus our deliberations about relativism and moral judgment were tied to concrete recommendations for public policy and were conducted in a public context that included participants from numerous adversarial legal proceedings.In tandem with our reconstruction of the past, we undertook three projects to examine the current state of human radiation experiments. First, we studied how each federal agency that currently conducts or funds research involving human subjects regulates and oversees its research activity. Second, from among the very large number of federally-supported research projects involving human subjects, we randomly selected 125 projects for closer scrutiny. We reviewed all available relevant documentation for each project in order to assess how well it appeared to protect the rights and interests of the participating subjects. Third... (shrink)

The origin of the wave properties of matter is discussed from the point of view of stochastic electrodynamics. A nonrelativistic model of a charged particle with an effective structure embedded in the random zeropoint radiation field reveals that the field induces a high-frequency vibration on the particle; internal consistency of the theory fixes the frequency of this jittering at mc2/ħ. The particle is therefore assumed to interact intensely with stationary zeropoint waves of this frequency as seen from its proper (...) frame of reference; such waves, identified here as de Broglie's phase waves, give rise to a modulated wave in the laboratory frame, with de Broglie's wavelength and phase velocity equal to the particle velocity. The time-independent equation that describes this modulated wave is shown to be the stationary Schrödinger equation (or the Klein-Gordon equation in the relativistic version). In a heuristic analysis appled to simple periodic cases, the quantization rules are recovered from the assumption that for a particle in a stationary state there must correspond a stationary modulation.Along an independent and complementary line of reasoning, an equation for the probability amplitude in configuration space for a particle under a general potential V(x) is constructed, and it is shown that under conditions derived from stochastic electrodynamics it reduces to Schrödinger's equation. This equation reflects therefore the dual nature of the quantum particles, by describing simultaneously the corresponding modulated waveand the ensemble of particles. (shrink)

We thank the commentators for their interesting and helpful feedback on our previously published target article (Svoboda and Irvine, 2014). One of our objectives in that article was to identify areas of uncertainty that would need to be addressed in crafting a just SRM compensation system. The commentators have indicated some possible ways of reducing such uncertainty. Although we cannot respond to all their points due to limitations of space, we wish to address here the more pressing criticisms the (...) commentators have offered. (shrink)

The massless Thirring model of a self-interacting ferinion field in a curved two-dimensional background spacetime is considered. The exact operator solution for the fields and the equation for the two-point function are given and used to examine the radiation emitted by a two-dimensional black hole. The radiation is found to be thermal in nature, confirming general predictions to this effect. We compute the particle spectrum of the Thirring fermions at finite temperature in Minkowski space and point out (...) errors in a previous attempt at this calculation. Finally we calculate the vacuum expectation value of the stress tensor in an arbitrary two-dimensional spacetime by exploiting the connection between the thermal Hawking radiation from a black hole and the value of the so-called conformal trace anomaly. The latter is also computed quite independently, using dimensional regularization, from general considerations of the renormalization group. (shrink)

Gravitomagnetic equations result from applying quaternionic differential operators to the energy–momentum tensor. These equations are similar to the Maxwell’s EM equations. Both sets of the equations are isomorphic after changing orientation of either the gravitomagnetic orbital force or the magnetic induction. The gravitomagnetic equations turn out to be parent equations generating the following set of equations: the vorticity equation giving solutions of vortices with nonzero vortex cores and with infinite lifetime; the Hamilton–Jacobi equation loaded by the quantum potential. This equation (...) in pair with the continuity equation leads to getting the Schrödinger equation describing a state of the superfluid quantum medium ; gravitomagnetic wave equations loaded by forces acting on the outer space. These waves obey to the Planck’s law of radiation. (shrink)

Complexified Liénard–Wiechert potentials simplify the mathematics of Kerr–Newman particles. Here we constrain them by fiat to move along Bohmian trajectories to see if anything interesting occurs, as their equations of motion are not known. A covariant theory due to Stueckelberg is used. This paper deviates from the traditional Bohmian interpretation of quantum mechanics since the electromagnetic interactions of Kerr–Newman particles are dictated by general relativity. A Gaussian wave function is used to produce the Bohmian trajectories, which are found to be (...) multi-valued. A generalized analytic continuation is introduced which leads to an infinite number of trajectories. These include the entire set of Bohmian trajectories. This leads to multiple retarded times which come into play in complex space-time. If one weights these trajectories by their natural Bohmian weighting factors, then it is found that the particles do not radiate, that they are extended, and that they can have a finite electrostatic self energy, thus avoiding the usual divergence of the charged point particle. This effort does not in any way criticize or downplay the traditional Bohmian interpretation which does not assume the standard electromagnetic coupling to charged particles, but it suggests that a hybridization of Kerr–Newman particle theory with Bohmian mechanics might lead to interesting new physics, and maybe even the possibility of emergent quantum mechanics. (shrink)

We apply a method analogous to the eikonal approximation to the Maxwell wave equations in an inhomogeneous anisotropic medium and geodesic motion in a three dimensional Riemannian manifold, using a method which identifies the symplectic structure of the corresponding mechanics, to the five dimensional generalization of Maxwell theory required by the gauge invariance of Stueckelberg's covariant classical and quantum dynamics. In this way, we demonstrate, in the eikonal approximation, the existence of geodesic motion for the flow of mass in a (...) four dimensional pseudo-Riemannian manifold. These results provide a foundation for the geometrical optics of the five dimensional radiation theory and establish a model in which there is mass flow along geodesics. We then discuss the interesting case of relativistic quantum theory in an anisotropic medium as well. In this case the eikonal approximation to the relativistic quantum mechanical current coincides with the geodesic flow governed by the pseudo-Riemannian metric obtained from the eikonal approximation to solutions of the Stueckelberg–Schrödinger equation. The locally symplectic structure which emerges is that of a generally covariant form of Stueckelberg's mechanics on this manifold. (shrink)

That space and time should be integrated into a single entity, spacetime, is the great insight of Einstein's special theory of relativity, and leads us to regard spacetime as a fundamental context in which to make sense of the world around us. But it is not the only one. Causality is equally important and at least as far as the special theory goes, it cannot be subsumed under a fundamentally geometrical form of explanation. In fact, the agent of propagation (...) of causal influence is electromagnetic radiation. In this examination, the authors find support for a rationalist approach to physics, never neglecting experimentation, but rejecting a simple empiricist or positivist view of science. (shrink)

In lieu of an abstract, here is a brief excerpt of the content:The Journal of Aesthetic Education 37.4 (2003) 32-41 [Access article in PDF] Does Art Education Dream of Disneyland? [Figures] Introduction What image can we present when challenged to illustrate art education in the form of a scheme? The word "illustration" literally means to build understanding through an explanatory diagram. In art education or anything [End Page 32] else, the use of a visual image to understand a certain system (...) can be interpreted as a question of human sensitivity and recognition. Translating minute nuances or peculiarities of information into a vibrant image is, however, a confusing and difficult exercise. In this essay, I attempt to portray those elements crucial to the teaching and learning process of art education using Disneyland as a structural as well as a functional metaphor. The Happiest Place on Earth? Disneyland is depicted as "a dream world" and "the happiest place on earth." As described in various incisive essays, Disneyland is a symbol of modern American culture, an ultimate form of the consumer society or the hegemony of entertainment. 1 To start with, the structural elements of this epitome of Walt Disney's vision are outlined.Walt Disney created Main Street USA (the World Bazaar) to make all visitors feel as if they are the leading character in a Disney film, walking through the main street of life. He attempted to remove the ugliness of everyday life from his dream space by eradicating the back streets of the real world. The design of the buildings along Main Street originates from Walt Disney's hometown. The sense of distance within the Disney complex is enhanced by using a smaller scale for the upper stories of buildings and a progressively narrowing street.Sleeping Beauty's Castle (or Cinderella Castle at Tokyo Disneyland) lies beyond Main Street and is modeled on Neuschwanstein Castle in Fussen,South Bayern, Germany. The road leading to the castle ascends slightly which amplifies the anticipation factor for visitors. Sleeping Beauty's Castle is the centerpiece of Disneyland and functions as the hub to guide visitors to various lands. Several attractive spaces radiate from this hub, forming a total of six areas.On the extension line from the Entrance via Sleeping Beauty's Castle lies Fantasyland where Walt Disney has reproduced the world of animation based on European legends and fables. Toontown lies beyond Fantasyland. This is a world of familiar characters, such as Mickey, Minnie, and Goofy. Traveling clockwise, Tomorrowland is next where all kinds of imaginary worlds await visitors. Adventureland, on the opposite side of Main Street, offers worlds of different cultures and spaces for adventure. Beyond Adventureland lies Westernland, designed to invite visitors to return to the Wild West.It is possible to form a hypothesis that there are three axes connecting the six lands. Those axes run through Sleeping Beauty's Castle that acts as the hub and two opposing areas on the same axis with the Castle being the point of symmetry.The first axis could be the axis of "reality." If Main Street is considered to be the "crawling approachway" from the everyday sphere to dreamland,Fantasyland, offering playful space of extraordinary imagination, is set [End Page 33] against the ordinary space for everyday life. The second axis is the axis of "relationship" which connects individual persons to society. Toontown presents a world of fraternity and is a place where people bonded by kinship or friendship can trust each other and feel at ease. Frontierland, located on the opposite side of this axis creates a solitary space where people leave family and friends for the adventure of traveling to unknown lands. The third and final axis is that of "time" from the past to the future. Tomorrowland is a future world based on fantasy and imagination where prophecies becomereality. On the opposite side of this axis lies Westernland embodying the history and traditions of the American past.It is possible to regard each area of Disneyland, structured by these different worlds, as a metaphor to reflect the basic content and structure of art education in the context of the general curriculum. In fact... (shrink)

In lieu of an abstract, here is a brief excerpt of the content:The Journal of Aesthetic Education 37.4 (2003) 32-41 [Access article in PDF] Does Art Education Dream of Disneyland? [Figures] Introduction What image can we present when challenged to illustrate art education in the form of a scheme? The word "illustration" literally means to build understanding through an explanatory diagram. In art education or anything [End Page 32] else, the use of a visual image to understand a certain system (...) can be interpreted as a question of human sensitivity and recognition. Translating minute nuances or peculiarities of information into a vibrant image is, however, a confusing and difficult exercise. In this essay, I attempt to portray those elements crucial to the teaching and learning process of art education using Disneyland as a structural as well as a functional metaphor. The Happiest Place on Earth? Disneyland is depicted as "a dream world" and "the happiest place on earth." As described in various incisive essays, Disneyland is a symbol of modern American culture, an ultimate form of the consumer society or the hegemony of entertainment. 1 To start with, the structural elements of this epitome of Walt Disney's vision are outlined.Walt Disney created Main Street USA (the World Bazaar) to make all visitors feel as if they are the leading character in a Disney film, walking through the main street of life. He attempted to remove the ugliness of everyday life from his dream space by eradicating the back streets of the real world. The design of the buildings along Main Street originates from Walt Disney's hometown. The sense of distance within the Disney complex is enhanced by using a smaller scale for the upper stories of buildings and a progressively narrowing street.Sleeping Beauty's Castle (or Cinderella Castle at Tokyo Disneyland) lies beyond Main Street and is modeled on Neuschwanstein Castle in Fussen,South Bayern, Germany. The road leading to the castle ascends slightly which amplifies the anticipation factor for visitors. Sleeping Beauty's Castle is the centerpiece of Disneyland and functions as the hub to guide visitors to various lands. Several attractive spaces radiate from this hub, forming a total of six areas.On the extension line from the Entrance via Sleeping Beauty's Castle lies Fantasyland where Walt Disney has reproduced the world of animation based on European legends and fables. Toontown lies beyond Fantasyland. This is a world of familiar characters, such as Mickey, Minnie, and Goofy. Traveling clockwise, Tomorrowland is next where all kinds of imaginary worlds await visitors. Adventureland, on the opposite side of Main Street, offers worlds of different cultures and spaces for adventure. Beyond Adventureland lies Westernland, designed to invite visitors to return to the Wild West.It is possible to form a hypothesis that there are three axes connecting the six lands. Those axes run through Sleeping Beauty's Castle that acts as the hub and two opposing areas on the same axis with the Castle being the point of symmetry.The first axis could be the axis of "reality." If Main Street is considered to be the "crawling approachway" from the everyday sphere to dreamland,Fantasyland, offering playful space of extraordinary imagination, is set [End Page 33] against the ordinary space for everyday life. The second axis is the axis of "relationship" which connects individual persons to society. Toontown presents a world of fraternity and is a place where people bonded by kinship or friendship can trust each other and feel at ease. Frontierland, located on the opposite side of this axis creates a solitary space where people leave family and friends for the adventure of traveling to unknown lands. The third and final axis is that of "time" from the past to the future. Tomorrowland is a future world based on fantasy and imagination where prophecies becomereality. On the opposite side of this axis lies Westernland embodying the history and traditions of the American past.It is possible to regard each area of Disneyland, structured by these different worlds, as a metaphor to reflect the basic content and structure of art education in the context of the general curriculum. In fact... (shrink)

Classical electron theory with classical electromagnetic zero-point radiation (stochastic electrodynamics) is the classical theory which most closely approximates quantum electrodynamics. Indeed, in inertial frames, there is a general connection between classical field theories with classical zero-point radiation and quantum field theories. However, this connection does not extend to noninertial frames where the time parameter is not a geodesic coordinate. Quantum field theory applies the canonical quantization procedure (depending on the local time coordinate) to a mirror-walled box, and, in (...) general, each non-inertial coordinate frame has its own vacuum state. In particular, there is a distinction between the “Minkowski vacuum” for a box at rest in an inertial frame and a “Rindler vacuum” for an accelerating box which has fixed spatial coordinates in an (accelerating) Rindler frame. In complete contrast, the spectrum of random classical zero-point radiation is based upon symmetry principles of relativistic spacetime; in empty space, the correlation functions depend upon only the geodesic separations (and their coordinate derivatives) between the spacetime points. The behavior of classical zero-point radiation in a noninertial frame is found by tensor transformations and still depends only upon the geodesic separations, now expressed in the non-inertial coordinates. It makes no difference whether a box of classical zero-point radiation is gradually or suddenly set into uniform acceleration; the radiation in the interior retains the same correlation function except for small end-point (Casimir) corrections. Thus in classical theory where zero-point radiation is defined in terms of geodesic separations, there is nothing physically comparable to the quantum distinction between the Minkowski and Rindler vacuum states. It is also noted that relativistic classical systems with internal potential energy must be spatially extended and can not be point systems. The classical analysis gives no grounds for the “heating effects of acceleration through the vacuum” which appear in the literature of quantum field theory. Thus this distinction provides (in principle) an experimental test to distinguish the two theories. (shrink)

Around 540 million years ago there was a sudden, dramatic adaptive radiation known as the Cambrian Explosion. This event marked the origin of almost all of the phyla (major lineages characterized by fundamental body plans) of animals that would ever live on earth, as well the appearance of many notable features such as rigid skeletons and other hard parts, complex jointed appendages, eyes, and brains. This radical evolutionary event has been a major puzzle for evolutionary biologists since Darwin, and (...) while our understanding of it has recently improved with new fossil finds, richer molecular phylogenies, and better grasp of ecological, evolutionary, and developmental processes generally, unanswered questions remain. In this paper I argue that a basic cognitive toolkit for embodied, object-oriented, spatial cognition (what I call Basic Cognitive Embodiment) is a practical necessity for control of a large, mobile, complexly articulated body in space. This hypothesis allows us to relate the complexification of animal bodies to the complexification of perception, cognition and behavior in a way that can help to fill in gaps in our emerging picture of the Cambrian Explosion, as well as shed light on the deep evolutionary origins of the mind. (shrink)

PROCESS this ordered movement of energy from one object to other object, changing their physical parameters. EVENT is the information on process. LIFE is the information on processes. The LIFE is process. The INFORMATION is a part of energy reflected or radiated by object written down in memory of the person, a material, space.

Prologue: Stormclouds : London, April 1900 -- Quantum of action: The most strenuous work of my life : Berlin, December 1900 ; Annus Mirabilis : Bern, March 1905 ; A little bit of reality : Manchester, April 1913 ; la Comédie Française : Paris, September 1923 ; A strangely beautiful interior : Helgoland, June 1925 ; The self-rotating electron : Leiden, November 1925 ; A late erotic outburst : Swiss Alps, Christmas 1925 -- Quantum interpretation: Ghost field : Oxford, August (...) 1926 ; All this damned quantum jumping : Copenhagen, October 1926 ; The uncertainty principle : Copenhagen, February 1927 ; The 'Kopenhagener geist' : Copenhagen, June 1927 ; There is no quantum world : Lake Como, September 1927 -- Quantum debate: The debate commences : Brussels, October 1927 ; An absolute wonder : Cambridge, Christmas 1927 ; The photon box : Brussels, October 1930 ; A bolt from the blue : Princeton, May 1935 ; The paradox of Schrödinger's cat : Oxford, August 1935 -- Interlude: The first war of physics : Christmas 1938-August 1945 -- Quantum fields: Shelter Island : Long Island, June 1947 ; Pictorial semi-vision thing : New York, January 1949 ; A beautiful idea : Princeton, February 1954 ; Some strangeness in the proportion : Rochester, August 1960 ; Three quarks for Muster Mark! : New York, March 1963 ; The 'God particle' : Cambridge, Massachusetts, Autumn 1967 -- Quantum particles: Deep inelastic scattering : Stanford, August 1968 ; Of charm and weak neutral currents : Harvard, February 1970 ; The magic of colour : Princeton/Harvard, April 1973 ; The November revolution : Long Island/Stanford, November 1974 ; Intermediate vector bosons : Geneva, January/June 1983 ; The standard model : Geneva, September 2003 -- Quantum reality: Hidden variable : Princeton, Spring 1951 ; Bertlmann's socks : Boston, September 1964 ; The Aspect experiments : Paris, September 1982 ; The quantum eraser : Baltimore, January 1999 ; Lab cats : Stony Brook/Delft, July 2000 ; The persistent illusion : Vienna, December 2006 -- Quantum cosmology: The wavefunction of the universe : Princeton, July 1966 ; Hawking radiation : Oxford, February 1974 ; The first superstring revolution : Aspen, August 1984 ; Quanta of space and time : Santa Barbara, February 1986 ; Crisis? What crisis? : Durham, Summer 1994 -- A quantum of solace? : Geneva, March 2010. (shrink)

In lieu of an abstract, here is a brief excerpt of the content:Editor's NoteErik DoxtaderThe freedom of conversation is being lost. … Warmth is ebbing from things.—Walter Benjamin, One-way StreetInsufficient data for a meaningful answer.—Multivac (Isaac Asimov, The Last Question)This issue of Philosophy & Rhetoric, a somewhat rare double-issue, features significant and inspiring work that moves in a variety of directions and proceeds in a number of idioms, while also responding directly and indirectly to a complex exigence, though perhaps in (...) a less familiar sense of the term, as what Giorgio Agamben calls a "messianic modality" that "coincides with the possibility of philosophy itself"—exigency as the expression of what remains unforgettable in the midst of all that is no longer remembered for the sake of history's progress. Appearing between contingency and necessity, exigency is not then a problem to be re-solved but the opening of a question; or more precisely, the epideictic expression of question-ability, the beginning of inquiry into what calls forth and perhaps even demands its possibility, for now.On what grounds do old questions stand? Through what power and by what happenstance are new questions found and formed? And when—in what kinds of moments do questions appear? With what force do they arrive? At what cost? What questions inflict violence? What violence thwarts a question? What do we (not) ask? How does the (un)questionable give way? Can multiple disciplines ever pose let alone inquire into the same question? What are the (de)constitutive elements of a good question? What does a good question do? Has pious genealogy corrupted the question? Does the discovery of a question remain one of the last "secrets," the unhinged authentic insight about which little can or should be said?A century ago, announcing the launch of Angelus Novus, Benjamin reflected on the moment and contended that the "vocation of a journal is to proclaim the spirit of its age." Such a task, in his view, demanded a strict "relevance to the present" even over "unity or clarity" and required exposing the "talented fakes" and resisting "the sterile pageant of new and fashionable events" that obscure how "impossible it is in our age to give a voice to [End Page 213] any communality [Gemeinsamkeit]." It is a tall and certainly debatable order, one that Benjamin himself was unable to realize—Angelus never got off the ground. But perhaps the underlying insight remains, the basic importance of holding space for work that discerns and expresses the potential of question-ability.This potential may well be the spirit-breath of an age. And, for now, here and now, it may well be a pressing question—on the shore of Ontario's Crawford Lake, waiting for official word that the Holocene has ended; in a largely unacknowledged transition, seemingly out of the pandemic's worst, ramping back up to speed, and yet deeply uncertain about the next normal; in the midst of the two "wars" (a term to which all participating parties will not agree) that make the front page (or the top of the feed) and the many that do not, the grotesque surfeit of increasingly automatic-droning violence unfolding on the grounds of sanctified rage that makes it difficult to ask let alone grasp what violence is; at the gates of the university, where so much inquiry is supplanted with so many strategic plans, and academic freedom is slowly juridified to the advantage of legislatures eager to rewrite the mission; and, in the midst of the noisy quietude that thwarts so many of the small inquiries into well-being that weave the fabric of public life.It's been a pleasure to work with all of those who have contributed to this issue of Philosophy & Rhetoric. Indeed, the pages that follow radiate with curiosity and insight. Together, they are an expression of inquiry in which question-ability remains unforgettable and there remains a moment to ask—after the question. [End Page 214]Copyright © 2024 The Pennsylvania State University... (shrink)

Intraspecific niche variation can differentially impact community processes and can represent the initial stages of adaptive radiation. Here we test for intraspecific differences in niche use in a keystone species, the alewife (Alosa pseudoharengus). To test whether feedbacks between predator foraging traits and prey communities have led to differences in niche use, we compare the diet composition and trophic position of anadromous and landlocked alewife populations. These populations differ in phenotypic traits related to foraging (gill raker spacing, gape width, (...) and prey selectivity). Trait differences appear to have resulted from eco-evolutionary feedbacks between alewives and their zooplankton prey, and suggest that these two life history forms are exploiting different niches. Direct diets show that anadromous alewives consume a greater biomass of predatory copepods than do landlocked alewives. Anadromous alewives also consume more ostracods—a littoral prey item—as the growing season progresses. These diet differences do not translate into a significant difference in trophic position, as estimated from stable isotopes. However, stable-isotope estimates of diet source show that during early fall, anadromous alewives obtain significantly more of their dietary carbon from the littoral food web. This increased reliance on littoral prey is likely a result of a diet switch that occurs in response to the alewife-driven exhaustion of large-bodied prey items available in the pelagic zone, i.e., alewife niche construction. These findings show the existence of important intraspecific niche differences in the alewife and support the role of eco-evolutionary feedbacks in shaping these niche differences. The initiation of alewife divergence is the result of dam building by humans. Therefore, alewife niche differentiation can be considered to be an eco-evolutionary byproduct of human cultural niche construction. (shrink)

A massless Weyl-invariant dynamics of a scalar, a Dirac spinor, and electromagnetic fields is formulated in a Weyl space, W4, allowing for conformal rescalings of the metric and of all fields with nontrivial Weyl weight together with the associated transformations of the Weyl vector fields κμ, representing the D(1) gauge fields, with D(1) denoting the dilatation group. To study the appearance of nonzero masses in the theory the Weyl symmetry is broken explicitly and the corresponding reduction of the Weyl (...) space W4 to a pseudo-Riemannian space V4 is investigated assuming the breaking to be determined by an expression involving the curvature scalar R of the W4 and the mass of the scalar, selfinteracting field. Thereby also the spinor field acquires a mass proportional to the modulus Φ of the scalar field in a Higgs-type mechanism formulated here in a Weyl-geometric setting with Φ providing a potential for the Weyl vector fields κμ. After the Weyl-symmetry breaking, one obtains generally covariant and U(1) gauge covariant field equations coupled to the metric of the underlying V4. This metric is determined by Einstein's equations, with a gravitational coupling constant depending on Φ, coupled to the energy momentum tensors of the now massive fields involved together with the (massless) radiation fields. (shrink)

Recently many methods for reducing the risk of human extinction have been suggested, including building refuges underground and in space. Here we will discuss the perspective of using military nuclear submarines or their derivatives to ensure the survival of a small portion of humanity who will be able to rebuild human civilization after a large catastrophe. We will show that it is a very cost-effective way to build refuges, and viable solutions exist for various budgets and timeframes. Nuclear submarines (...) are surface independent, and could provide energy, oxygen, fresh water and perhaps even food for their inhabitants for years. They are able to withstand close nuclear explosions and radiation. They are able to maintain isolation from biological attacks and most known weapons. They already exist and need only small adaptation to be used as refuges. But building refuges is only “Plan B” of existential risk preparation; it is better to eliminate such risks than try to survive them. (shrink)

Becoming is interpreted by various sciences. The exact sciences, physics, and chemistry, interpret this universal becoming or change of all things on the model of mathematical equations. In such an equation of quantities or magnitudes, one side always balances the other. We call such a process “circular”. Numbers may be subdivided or contracted, they may change their places or positions, but the sum total of the whole equation remains immutably the same. In this manner mechanics constructs change as a change (...) of positions of unchanging particles in a continuous but divisible space and in a continuous but divisible time. Chemistry constructs qualitative change as a change of unchanging elements in such a fashion that the sum total of the elements involved in such transactions is always completely accounted for. But in the twentieth century becoming entered these closed systems. There are no unchanging atoms now, and no unchanging chemical elements. Both the physical atom and the chemical element, thought immutable before, are now seen to disintegrate, to radiate, to change their character according to their position in the “field” of energy in which they occur. (shrink)

The concept of time is examined using the second law of thermodynamics that was recently formulated as an equation of motion. According to the statistical notion of increasing entropy, flows of energy diminish differences between energy densities that form space. The flow of energy is identified with the flow of time. The non-Euclidean energy landscape, i.e. the curved space–time, is in evolution when energy is flowing down along gradients and levelling the density differences. The flows along the steepest (...) descents, i.e. geodesics are obtained from the principle of least action for mechanics, electrodynamics and quantum mechanics. The arrow of time, associated with the expansion of the Universe, identifies with grand dispersal of energy when high-energy densities transform by various mechanisms to lower densities in energy and eventually to ever-diluting electromagnetic radiation. Likewise, time in a quantum system takes an increment forwards in the detection-associated dissipative transformation when the stationary-state system begins to evolve pictured as the wave function collapse. The energy dispersal is understood to underlie causality so that an energy gradient is a cause and the resulting energy flow is an effect. The account on causality by the concepts of physics does not imply determinism; on the contrary, evolution of space–time as a causal chain of events is non-deterministic. (shrink)

Some scientists suggest that it might be possible to reflect a portion of incoming sunlight back into space to reduce climate change and its impacts. Others argue that such solar radiation management (SRM) geoengineering is inherently incompatible with democracy. In this article, we reject this incompatibility argument. First, we counterargue that technologies such as SRM lack innate political characteristics and predetermined social effects, and that democracy need not be deliberative to serve as a standard for governance. We then (...) rebut each of the argument’s core claims, countering that (1) democratic institutions are sufficiently resilient to manage SRM, (2) opting out of governance decisions is not a fundamental democratic right, (3) SRM may not require an undue degree of technocracy, and (4) its implementation may not concentrate power and promote authoritarianism. Although we reject the incompatibility argument, we do not argue that SRM is necessarily, or even likely to be, democratic in practice. (shrink)