Faith and Citizenship in a Global Context

Faith and Citizenship in a Global Context

In this panel discussion led by Yale Law School Dean Harold Koh, activists, academicians and former diplomats covered subjects that included the international community’s inability to intervene in Darfur, citizenship in the face of globalization, and to what extent religion informs U.S. foreign policy. Panelists included Jennifer Butler, Executive Director, Faith in Public Life; Heidi Hadsell, President, Hartford Seminary; James Joseph, U.S. Ambassador to South Africa, 1996-99 and Professor of the Practice of Public Policy, Sanford Institute of Public Policy, Duke University ; Paul Lakeland, Professor of Religious Studies at Fairfield University; James Laney, U.S. Ambassador to South Korea, 1993-97; and Emilie Townes, Andrew W. Mellon Professor of African American Religion and Theology at Yale Divinity School. (May 4, 2007)

Faith and Citizenship in America

Faith and Citizenship in America

In this panel discussion led by Yale Law School Professor Harlon Dalton, academicians, journalists and activists examined the intersection between faith and politics in American life. Panelists included Randall Balmer, Ann Whitney Olin Professor of American Religion, Barnard College; Serene Jones, Titus Street Professor of Theology, Yale Divinity School ; Michael Kieschnick, President and Co-founder, Working Assets; Peter Laarman, Executive Director, Progressive Christians Uniting; David Price, Democratic U.S. Representative, North Carolina; and Amy Sullivan, Contributing Editor, The Washington Monthly. (May 4, 2007)

Pastoral Care versus Inappropriate Religious Proselytizing

Pastoral Care versus Inappropriate Religious Proselytizing

Kristen Leslie, Associate Professor of Pastoral Care and Counseling at Yale Divinity SchoolKristen Leslie, Associate Professor of Pastoral Care & Counseling at Yale Divinity School, discusses sexual assault in the United States Air Force Academy and the subsequent religious intolerance of chaplains at the Academy.

24 – The Multiverse and Theories of Everything

24 – The Multiverse and Theories of Everything

Professor Bailyn begins the class with a discussion of a recent New York Times article about the discovery of a new, earth-like planet. He then discusses concepts such as epicycles, dark energy and dark matter; imaginary ideas invented to explain 96% of the universe. The Anthropic Principle is introduced and the possibility of the multiverse is addressed. Finally, biological arguments are put forth for how complexity occurs on a cosmological scale. The lecture and course conclude with a discussion on the fine differences between science and philosophy.

23 – Other Constraints: The Cosmic Microwave Background

23 – Other Constraints: The Cosmic Microwave Background

Reasons for the expansion of the universe are addressed at the start of this lecture, focusing especially on the acceleration of dark energy. Supernovae were the first evidence for the existence of dark energy. Two other proofs are presented. The first is the Cosmic Microwave Background, which is a form of electromagnetic radiation that is perfectly smooth and equal in all directions. It firmly supports the Big Bang theory. Projects attempting to measure it, such as COBE and WMAP, are discussed. Secondly, Large-Scale Clustering is introduced: by measuring the degree of clustering, astronomers hope to advance their understanding of dark energy and dark matter. Computer simulations of the evolution of the universe are shown.

22 – Supernovae

22 – Supernovae

Professor Bailyn offers a review of what is known so far about the expansion of the universe from observing galaxies, supernovae, and other celestial phenomena. The rate of the expansion of the universe is discussed along with the Big Rip theory and the balance of dark energy and dark matter in the universe over time. The point at which the universe shifts from accelerating to decelerating is examined. Worries related to the brightness of high redshift supernovae and the effects of gravitational lensing are explained. The lecture also describes current project designs for detecting supernovae at high or intermediate redshift, such as the Joint Dark Energy Mission (JDEM) and Large Synoptic Survey Telescope (LSST).

21 – Dark Energy and the Accelerating Universe and the Big Rip

21 – Dark Energy and the Accelerating Universe and the Big Rip

Class begins with a review of the mysterious nature of dark matter, which accounts for three quarters of the universe. Different models of the universe are graphed. The nature, frequency, and duration of supernovae are then addressed. Professor Bailyn presents data from the Supernova Cosmology Project and pictures of supernovae taken by the Hubble Space Telescope. The discovery of dark energy is revisited and the density of dark energy is calculated. The Big Rip is presented as an alternative hypothesis for the fate of the universe.

20 – Dark Matter

20 – Dark Matter

This lecture introduces an important concept related to the past and future of the universe: the Scale factor, which is a function of time. With reference to a graph whose coordinates are the Scale factor and time, the problem of dark matter is addressed again. Cosmological redshifts are measured to determine the scale of the universe. The discovery of the repulsive, anti-gravitational force of dark energy is explained. The lecture concludes with discussion of Einstein’s biggest mistake: the invention of the cosmological constant to balance gravity.

19 – Omega and the End of the Universe

19 – Omega and the End of the Universe

Class begins with a review of the issues previously addressed about the origin and fate of the universe. The role of gravity in the expansion of the universe is discussed and given as the reason why the rate of expansion cannot remain constant and will eventually slow down. The actual density of the universe is calculated using various methods. Finally, the unsolved problem of dark matter is addressed and two explanatory hypotheses are proposed. One is that the universe is comprised of WIMPs (Weakly Interactive Massive Particles) that fulfill two requirements: they have mass and do not interact with light. The second hypothesis is that dark matter is made of MACHOs (Massive Astrophysical Compact Halo Objects), which scientists have attempted to identify through gravitational lenses.

18 – Hubble’s Law and the Big Bang pt 3

18 – Hubble’s Law and the Big Bang pt 3

Professor Bailyn returns to the subject of the expansion of the universe to offer explanations that do not require belief in the Big Bang theory. One alternative is a theory that, in the past, the entire universe was reduced to an “initial singularity,” in which everything was much closer, and therefore denser and hotter. Since the universe is in constant flux, however, it follows that in the future things will drift apart. The Steady State explanation for the expansion of the universe is then explained. Coined as a derogatory term meant to ridicule supporters of the Big Bang theory, Steady State purports that new energy and matter are constantly created as the universe expands, to fill in the void that results from the expansion. The discovery of quasars refuted the Steady State theory. The lecture ends with a discussion of how observing very distant objects allows us to look back in time, and also gives us a glimpse into the future of galaxies and the universe.