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Prateek Agrawal

Researcher at Harvard University

Publications -  78
Citations -  5360

Prateek Agrawal is an academic researcher from Harvard University. The author has contributed to research in topics: Dark matter & Axion. The author has an hindex of 34, co-authored 67 publications receiving 4258 citations. Previous affiliations of Prateek Agrawal include University of Maryland, College Park & Fermilab.

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On the Cosmological Implications of the String Swampland

TL;DR: In this paper, the authors study constraints imposed by two proposed string Swampland criteria on cosmology and find that inflationary models are generically in tension with these two criteria, and they argue that the universe will undergo a phase transition within a few Hubble times.
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FCC-ee: The Lepton Collider: Future Circular Collider Conceptual Design Report Volume 2

A. Abada, +1494 more
TL;DR: In this article, the authors present the second volume of the Future Circular Collider Conceptual Design Report, devoted to the electron-positron collider FCC-ee, and present the accelerator design, performance reach, a staged operation scenario, the underlying technologies, civil engineering, technical infrastructure, and an implementation plan.
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FCC-hh: The Hadron Collider

A. Abada, +1499 more
TL;DR: In this paper, the authors describe the detailed design and preparation of a construction project for a post-LHC circular energy frontier collider in collaboration with national institutes, laboratories and universities worldwide, and enhanced by a strong participation of industrial partners.
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FCC Physics Opportunities: Future Circular Collider Conceptual Design Report Volume 1

A. Abada, +1504 more
TL;DR: In this article, the physics opportunities of the Future Circular Collider (FC) were reviewed, covering its e+e-, pp, ep and heavy ion programs, and the measurement capabilities of each FCC component, addressing the study of electroweak, Higgs and strong interactions.
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Relic abundance of dark photon dark matter

TL;DR: In this paper, a new mechanism for producing the correct relic abundance of dark photon dark matter over a wide range of its mass, extending down to 10 − 20 eV, is presented.