Stanford Advisors

Contact

  • Academic
    ehtanin@stanford.edu
    University - Scholar Department: Physics Position: Postdoctoral Scholar

Additional Info

  • Mail Code: 4060

All Publications

  • Thermal damping of mass-modulating scalars PHYSICAL REVIEW D Banerjee, A., Nguyen, N. H., Tanin, E. H. 2026; 114 (1)

    View details for DOI 10.1103/rqq9-1dc2

    View details for Web of Science ID 001834431800001

  • Gravothermal pileup of collisional dark matter around compact objects PHYSICAL REVIEW D Ebadi, R., Tanin, E. H. 2026; 113 (5)

    View details for DOI 10.1103/qspg-rgh1

    View details for Web of Science ID 001711168200002

  • Direct deflection of Millicharged radiation JOURNAL OF HIGH ENERGY PHYSICS Berlin, A., Rajendran, S., Ramani, H., Tanin, E. H. 2025

    View details for DOI 10.1007/JHEP04(2025)198

    View details for Web of Science ID 001476745700005

  • LISA double white dwarf binaries as Galactic accelerometers PHYSICAL REVIEW D Ebadi, R., Strokov, V., Tanin, E. H., Berti, E., Walsworth, R. L. 2025; 111 (4)

    View details for DOI 10.1103/PhysRevD.111.044023

    View details for Web of Science ID 001452495000010

  • Indirect searches for ultraheavy dark matter in the time domain PHYSICAL REVIEW D Kaplan, D. E., Luo, X., Nguyen, N. H., Rajendran, S., Tanin, E. H. 2025; 111 (2)

    View details for DOI 10.1103/PhysRevD.111.023041

    View details for Web of Science ID 001410609500007

  • Fireball antinucleosynthesis PHYSICAL REVIEW D Fedderke, M. A., Kaplan, D. E., Mathur, A., Rajendran, S., Tanin, E. H. 2024; 109 (12)

    View details for DOI 10.1103/PhysRevD.109.123028

    View details for Web of Science ID 001288604300001

  • Dark Solar Wind PHYSICAL REVIEW LETTERS Chang, J., Kaplan, D. E., Rajendran, S., Ramani, H., Tanin, E. H. 2022; 129 (21): 211101

    Abstract

    We study the solar emission of light dark sector particles that self-interact strongly enough to self-thermalize. The resulting outflow behaves like a fluid which accelerates under its own thermal pressure to highly relativistic bulk velocities in the solar system. Compared to the ordinary noninteracting scenario, the local outflow has at least ∼10^{3} higher number density and correspondingly at least ∼10^{3} lower average energy per particle. We show how this generic phenomenon arises in a dark sector composed of millicharged particles strongly self-interacting via a dark photon. The millicharged plasma wind emerging in this model has novel yet predictive signatures that encourages new experimental directions. This phenomenon demonstrates how a small step away from the simplest models can lead to radically different outcomes and thus motivates a broader search for dark sector particles.

    View details for DOI 10.1103/PhysRevLett.129.211101

    View details for Web of Science ID 000886221300005

    View details for PubMedID 36461962