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Title: The High Energy X-ray Probe (HEX-P): supernova remnants, pulsar wind nebulae, and nuclear astrophysics

Journal Article · · Frontiers in Astronomy and Space Sciences
 [1];  [2];  [3];  [3];  [4];  [5];  [6];  [2];  [7];  [5];  [8];  [9];  [10];  [11];  [12];  [3];  [13];  [11];  [2];  [14] more »;  [15];  [11];  [16];  [17];  [17];  [18];  [19];  [20];  [21];  [22];  [11];  [23] « less
  1. North Carolina State University, Raleigh, NC (United States)
  2. Chungbuk National Univ., Cheongju (Korea, Republic of)
  3. New York Univ. (NYU), Abu Dhabi (United Arab Emirates)
  4. Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
  5. Columbia Univ., New York, NY (United States)
  6. Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States). Kavli Institute for Astrophysics and Space Research
  7. Saitama Univ. (Japan); Japan Aerospace Exploration Agency (ISAS/JAXA), Sagamihara, Kanagawa (Japan). Institute of Space and Astronautical Science
  8. Univ. of Tokyo (Japan)
  9. Univ. of Delaware, Newark, DE (United States)
  10. Univ. of Chicago, IL (United States)
  11. NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States)
  12. Univ. Paris Cité (France); Centre National de la Recherche Scientifique (CNRS), Paris (France)
  13. California Institute of Technology (CalTech), Pasadena, CA (United States)
  14. Univ. of Maryland, College Park, MD (United States)
  15. Univ. of Manitoba, Winnipeg, MB (Canada)
  16. Centre National de la Recherche Scientifique (CNRS), Annecy-le-Vieux (France); Univ. Savoie Mont Blanc, Annecy-le-Vieux (France)
  17. Saitama Univ. (Japan)
  18. Istituto Nazionale di Astrofisica (INAF), Firenze (Italy). Osservatorio Astrofisico di Arcetri; Istituto Nazionale di Astrofisica (INAF), Palermo (Italy). Osservatorio Astronomico di Palermo
  19. Meiji Univ., Kanagawa (Japan)
  20. Barnard College, New York, NY (United States)
  21. California Institute of Technology (CalTech), Pasadena, CA (United States). Jet Propulsion Laboratory (JPL)
  22. Kanagawa Univ., Yokohama, Kanagawa (Japan)
  23. Univ. of California, Berkeley, CA (United States)

HEX-P is a probe-class mission concept that will combine high spatial resolution X-ray imaging (< 10" full width at half maximum) and broad spectral coverage (0.2–80 keV) with an effective area far superior to current facilities (including XMM-Newton and NuSTAR) to enable revolutionary new insights into a variety of important astrophysical problems. HEX-P is ideally suited to address important problems in the physics and astrophysics of supernova remnants (SNRs) and pulsar wind nebulae (PWNe). For shell SNRs, HEX-P can greatly improve our understanding via more accurate spectral characterization and localization of non-thermal X-ray emission from both non-thermal-dominated SNRs and those containing both thermal and non-thermal components, and can discover previously unknown non-thermal components in SNRs. Multi-epoch HEX-P observations of several young SNRs (e.g., Cas A and Tycho) are expected to detect year-scale variabilities of X-ray filaments and knots, thus enabling us to determine fundamental parameters related to diffusive shock acceleration, such as local magnetic field strengths and maximum electron energies. For PWNe, HEX-P will provide spatially-resolved, broadband X-ray spectral data separately from their pulsar emission, allowing us to study how particle acceleration, cooling, and propagation operate in different evolution stages of PWNe. HEX-P is also poised to make unique and significant contributions to nuclear astrophysics of Galactic radioactive sources by improving detections of, or limits on, 44Ti in the youngest SNRs and by potentially discovering rare nuclear lines as evidence of double neutron star mergers. Throughout the paper, we present simulations of each class of objects, demonstrating the power of both the imaging and spectral capabilities of HEX-P to advance our knowledge of SNRs, PWNe, and nuclear astrophysics.

Research Organization:
Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
Sponsoring Organization:
USDOE National Nuclear Security Administration (NNSA); USDOE Laboratory Directed Research and Development (LDRD) Program; National Research Foundation of Korea (NRF); Japan Society for the Promotion of Science (JSPS)
Grant/Contract Number:
89233218CNA000001
OSTI ID:
2406634
Report Number(s):
LA-UR--23-33254
Journal Information:
Frontiers in Astronomy and Space Sciences, Journal Name: Frontiers in Astronomy and Space Sciences Vol. 10; ISSN 2296-987X
Publisher:
Frontiers Research FoundationCopyright Statement
Country of Publication:
United States
Language:
English

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