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Raman’s Re-election Campaign: A Test for Progressives

As Nithya Raman fights for reelection in a test for progressives, the race for the Hollywood Hills on the Los Angeles City Council has become the center of attention once again. Four years ago, Raman and her opponent sparred over who had the strongest credentials as political progressives, with Raman eventually emerging victorious as the first member of the Democratic Socialists of America to oust an incumbent at City Hall.

Now, as she seeks a second term in Tuesday’s election, Raman faces a more complex political landscape. Two opponents are challenging her, some activists criticize her from the left, and a surge of outside money has made it the most expensive L.A. City Council contest this year. The outcome of the race, with over $2.6 million in total spending, will impact the future of the progressive vision embraced by Raman and her allies at City Hall.

Councilmember Hugo Soto-Martínez noted that this vision includes measures to reduce evictions, expand renter relocation payments, and launch transportation initiatives. Raman, a self-proclaimed “pragmatic progressive,” has supported all these efforts and has been a champion on tenant issues, homelessness, and housing.

On the other hand, her opponent, Deputy City Atty. Ethan Weaver, describes himself as a “pragmatic Democrat” and criticizes Raman for being too far left on key issues like homelessness and public safety. Weaver emphasizes his support for laws against homeless encampments near schools and police raises to boost recruitment.

Despite criticism, Raman continues to support Inside Safe and other compassionate efforts while focusing on making LAHSA more effective in addressing homelessness. The race has attracted unprecedented financial support, with police and firefighter unions backing Weaver and Raman being targeted for her stance against special interests.

As the election nears, both candidates are making their case to voters. Raman highlights her record on tenant protections and homelessness reduction, citing drops in crime rates in her district. Weaver, however, paints a different picture, pointing out ongoing concerns about homelessness and personal safety.

The presence of a third candidate, Levon Baronian, adds another dimension to the race, making a November runoff more likely. While the campaigns have been marked by heavy spending and outside influences, each candidate is striving to connect with voters and secure their support.

Ultimately, the election will determine the course of progressive politics in L.A. and the future of the Hollywood Hills district. As Raman fights to retain her seat, the outcome will have far-reaching implications for the city and its residents. Whether voters opt for continuity with Raman or a change with Weaver, the decision will shape the trajectory of the council and its policies for the years to come.

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Further Support for Gravitational Wave Background in the Universe

The discovery of the gravitational wave background in 2016 marked a significant milestone in our understanding of the Universe. This groundbreaking discovery was further validated by the release of a second data set from the European Pulsar Timing Array, along with the addition of data from the Indian Pulsar Timing Array. These complementary studies have provided more evidence for the existence of the gravitational wave background, shedding light on the cosmic phenomena that shape our universe.

Gravitational waves are ripples in spacetime that are generated by violent processes such as merging black holes and colliding neutron stars. Predicted by Einstein in 1916 as part of his General Theory of Relativity, these waves have the ability to travel through space, largely unimpeded by any obstacles in their path. The first detection of gravitational waves in 2015 by the Laser Interferometer Gravitational-Wave Observatory (LIGO) confirmed their existence, originating from a gravitational merger between two black holes located 1.3 billion light years away.

The Laser Interferometer Gravitational-Wave Observatory is made up of two detectors, this one in Livingston, La., and one near Hanford, Wash. The detectors use giant arms in the shape of an “L” to measure tiny ripples in the fabric of the universe. Credit: Caltech/MIT/LIGO Lab

The recent confirmation of the gravitational wave background by the European and Indian Pulsar Timing Arrays indicates that we are detecting a combined signal from the mergers of supermassive black holes. This random distribution of gravity waves that permeates the Universe offers a new avenue for studying the cosmos, akin to the Cosmic Background Radiation. The collaborative efforts of various observatories and research institutions have enabled us to delve deeper into the mysteries of the Universe.

The full-sky image of the temperature fluctuations (shown as color differences) in the cosmic microwave background, made from nine years of WMAP observations. These are the seeds of galaxies, from a time when the universe was under 400,000 years old. Credit: NASA/WMAP

Utilizing pulsar timing arrays as galaxy-sized detectors, researchers have been able to monitor and analyze the pulse arrival times of galactic pulsars on Earth. By detecting subtle patterns in these signals, they can uncover the presence of the gravitational wave background. The latest study led by J. Antoniadis from the Institute of Astrophysics in Greece delves into the implications of the low-frequency signals observed in the recent data releases from various pulsar timing array systems.

The accumulation of data from multiple sources has provided undeniable evidence for the existence of the gravitational wave background. With ongoing Pulsar Timing Array projects, the signals of the low-frequency gravity waves will become more distinct, offering a wealth of opportunities to explore the Universe in this novel way. The focus now shifts towards interpreting these signals to unlock the secrets of the cosmos.

Source : The second data release from the European Pulsar Timing Array: IV. Implications for massive black holes, dark matter and the early Universe

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